Constellation Perseus (Hero)
Properties
Perseus lies east of Andromeda and southeast of Cassiopeia. The band of the Milky Way runs through this constellation and is darkened there by a large cloud of dust. Despite its glorious legend, Perseus is a figuratively difficult to understand constellation. The most striking is the small, elongated group of stars around Algenib. To the south of this is the bright, short-period variable star Algol, which is therefore also called devil's eye and represents the severed Medusa head. The area of the constellation is 615 square degrees and the center culminates around midnight on November 7th. [9, 15]
Stars with Proper Names:
- α Per: Mirphak, Mirfak, Marfak, Algenib
- β Per: Algol, Gorgona, Gorgonea Prima, Demon Star, El Ghoul
- η Per: Miram
- ξ Per: Menkib, Menkhib, Menchib
- ο Per: Atik, Ati, Al Atik
- π Per: Gorgonea Secunda
- ρ Per: Gorgonea Tertia
- ω Per: Gorgonea Quarta
Deep-Sky Object Descriptions
Mythology and History
Akrisios was the king of Argos and had a lovely daughter named Danae. The Oracle of Delphi prophesied that his grandson would one day kill him. For fear of this oracle, Akrisios had his daughter Danae locked in a tower so that she could not receive a husband. Of course, Akrisios could not have known that Zeus himself wanted to approach the lovely Danae. Zeus did this too and took the form of a golden rain that penetrated through the walls, joints, cracks and windows. Danae gave birth to a son, who was called "The one who emerged from flowing gold" or "The one who was born in gold" - Perseus. Akrisios didn’t keep this hidden for long, of course, and had his daughter and grandchild nailed into a box, which was then thrown into the sea.
Danae and Perseus drifted for a long time until they finally stranded on the coast of the stony island of Seriphos and were freed from their prison. On this island, Polydektes ruled, who soon campaigned for the beautiful Danae for years, but in vain. Either to force Danae into marriage after all, or to get Perseus out of the way, he sent Danae's son, who had meanwhile grown into a youth, to do a deadly task. He should get the head of Medusa.
Medusa was one of the Gorgons, one of the three daughters of Phorkys, who were equipped with snake hair and could cast a petrifying look. Two of these daughters were immortal, while Medusa was mortal. This father also had three other daughters, the Graien, "the ancient ones", who all together had only one eye and one tooth, which they had to borrow alternately if needed.
With the help of Hermes' winged shoes, the hat of Hades, which spread the impenetrable night, and the sickle sword of the limping fire and blacksmith god Hephaestus, Perseus succeeded in overcoming the Graien. He took away their only eye when the second of the three sisters wanted to see something. The way was cleared and he penetrated the Gorgons with the Hades cap pulled over his head. Perseus was careful not to look directly at Medusa, but only to look at her reflection in his polished shield - otherwise he would have immediately turned to stone. In this way he managed to behead Medusa, who was pregnant by Poseidon. The winged horse Pegasus then rose from the dead body. Even the grown-up warrior Chrysaor with a golden sword in hand emerged from her dead body. Perseus put the Gorgon head, which was still dripping with blood, into the magic sack and escaped with the help of the Hades cap, which spread deep darkness all around.
Perseus passed the coast of Ethiopia on his way back. There was the beautiful Andromeda - the daughter of the queen Kassiopeia and the king Kepheus - helpless and almost naked, only wearing a few pieces of jewelry, chained to a rock. A dreadful sea monster approached her with the intention of devouring her. Perseus immediately fell in love with the beautiful princess. He seized the opportunity and asked Andromedas father, King Cepheus of Ethiopia, that Hand of his daughter and a kingdom of her own to save her. He agreed, fearing for his daughter's life. Then Perseus put on his winged shoes and hurried through the air in the direction of sea monsters. Everything he did was designed to get this girl's attention to himself. The liberation took place only armed with the sword. [20] More common, however, is the variant in which he took Medusa's head out of the sack and petrified the sea monster into a rock in the sea. [66]
Perseus hurried back to his home island Seriphos and appeared in front of Polydectes. He shouted: "Here is your present!" and held up Medusa's head. Instantly the king and his followers froze to stone. Perseus returned to his lover Andromeda and married her. Both lived long and happily and had many children. One of her great-grandchildren was Hercules. When Perseus died, he was granted a place under the stars in the sky: his sword stretched up and the diabolical head of Medusa held in the other hand, so that she might look upon humanity for all time. [66]
Some names like Perseus, Perseus et Caput Medusae, Victor Gorgonei monstri, Gorgonifer are reminiscent of the story and Bearer of Medusa Head. This star formation was also transformed into biblically oriented images such as David with the head of Goliath and Apostle Paul with sword and book. [20]
Catalogs
| HR | B | F | DM | HD | SAO | FK5 | IR | M* | ADS | VarID | RA | Dec | vMag | spType | dMag | Sep ["] | Remarks |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| HR 470 | BD+53 363 | 10110 | 22493 | I | 01 40 13.1 | +53 52 06 | 6.39 | K5III | |||||||||
| HR 496 | φ | BD+49 444 | 10516 | 22554 | 57 | I | Phi Per | 01 43 39.6 | +50 41 19 | 4.07 | B2Vep | G:In neutral hydrogen region; Cas-Tau OB1.,P:Intrinsic polarization, probably due to circumstellar matter.,S:FeII, H in emission. Also classified B0nne, B1III-Vpe.,SB:126.696d. Primary, 16.8k/s, V0 -8.4k/s, msin3i 21.1, asini 29.2; secondary K 105.3k/s, sin3i 3.4,,SB:asini 184. Unresolved by speckle interferometry. Both components appear to be shell stars, B2Ve and B3Ve. Speculation,SB:that secondary is the helium core of a once more massive star whose mass was transferred to the primary.,VAR:Gamma Cas 4.03 - 4.11V, 19.5d. Amp. varies in per. 127d. Possible mass loss. Expanding circumstellar shell. | |||||
| HR 526 | BD+47 508 | 11031 | 37536 | 1438 | 01 49 15.7 | +47 53 49 | 5.82 | A3V | 0.7 | 1.9 | D:Component C 8.4v at 21", D 10.2v at 137".,SB:ADS 1438B. | ||||||
| HR 529 | BD+51 416 | 11151 | 22678 | 01 50 57.1 | +51 56 00 | 5.90 | F5IV | ||||||||||
| HR 533 | 1 | BD+54 396 | 11241 | 22690 | 2122 | V436 Per | 01 51 59.3 | +55 08 51 | 5.52 | B1.5V | G:In neutral hydrogen region; Cas-Tau OB1.,SB:15.6d, K 10k/s, V0 -9k/s.,VAR:E? 5.46 - 5.68y. | ||||||
| HR 536 | 2 | BD+50 379 | 11291 | 22696 | 1052 | 01 52 09.4 | +50 47 34 | 5.79 | B9IIIpHgMn | SB:5.6270d, K 26.5k/s, V0 +11.4k/s, asini 2.05. | |||||||
| HR 538 | BD+50 381 | 11335 | 22705 | 01 52 50.8 | +51 28 29 | 6.26 | A3V | ||||||||||
| HR 540 | BD+54 408 | 11408 | 22716 | 01 53 48.5 | +55 35 53 | 6.45 | A5m | ||||||||||
| HR 568 | 3 | BD+48 576 | 11949 | 37665 | 01 58 33.6 | +49 12 15 | 5.69 | K0IV | |||||||||
| HR 590 | 4 | BD+53 439 | 12303 | 22859 | 1054 | 02 02 18.1 | +54 29 15 | 5.04 | B8III | ||||||||
| HR 618 | BD+57 494 | 12953 | 22959 | V472 Per | 02 08 40.5 | +58 25 25 | 5.67 | A1Ia t | G:NGC 869; Per OB1.,S:Shell star.,VAR:Amp. 0.065V. Sp. var., H alpha profile var. | ||||||||
| HR 621 | BD+53 460 | 13137 | 22993 | 2146 | 02 10 07.8 | +53 50 35 | 6.31 | G8III | |||||||||
| HR 627 | 5 | BD+56 438 | 13267 | 23011 | 1685 | Var? | 02 11 29.0 | +57 38 45 | 6.36 | B5Ia | 6.9 | 60.0 | D:B, mag. diff 6.9v at 5.6".,G:Per OB1; h Per. | ||||
| HR 641 | BD+57 519 | 13476 | 23044 | 02 13 41.5 | +58 33 40 | 6.44 | A3Iab | G:Per OB1; h Per. | |||||||||
| HR 654 | BD+56 471 | 13854 | 23115 | W | Var? | 02 16 51.7 | +57 03 19 | 6.48 | B1Iab e | 0.9 | 103.0 | G:NGC 869 = h Per; Per OB1. | |||||
| HR 661 | 8 | BD+57 535 | 13982 | 23143 | 2157 | 02 17 59.9 | +57 53 59 | 5.75 | K3III | ||||||||
| HR 662 | 7 | BD+56 486 | 13994 | 23149 | 1753 | 02 18 04.5 | +57 31 00 | 5.98 | G7III | 2.6 | 121.9 | C:Heavily reddened.,G:May not be member of Per OB2.,N:Sometimes misidentified as Chi Per. | |||||
| HR 685 | 9 | BD+55 598 | 14489 | 23256 | 2159 | 1802 | V474 Per | 02 22 21.4 | +55 50 44 | 5.17 | A2Ia v | 7.8 | 11.6 | D:Fixed.,G:Per OB1.,RV:Var. in period over 200d.,S:Shell star.,VAR:Amp. 0.05V. Sp. and H alpha profile var. | |||
| HR 690 | BD+54 535 | 14662 | 23283 | 1820 | V440 Per | 02 23 51.8 | +55 21 52 | 6.28 | F7Ib | 8.1 | 10.0 | VAR:CDelta, amp. 0.123V, 7.572d. | |||||
| HR 696 | 10 | BD+55 612 | 14818 | 23304 | Var | 02 25 16.0 | +56 36 36 | 6.25 | B2Ia e | G:Per OB1; in cluster Chi Per; NGC 884.,VAR:Amp. at 0.58 micrometers about 0.15m. | |||||||
| HR 716 | BD+54 557 | 15253 | 23369 | 1878 | 02 29 25.0 | +55 32 11 | 6.51 | A2pShell v | 1.3 | 2.8 | D:Companion A3IV.,VAR:ADS 1878A, spectrum variable, shell star. | ||||||
| HR 785 | 11 | BD+54 598 | 16727 | 23555 | 2188 | 02 43 02.8 | +55 06 21 | 5.77 | B7IIIpHg | SB:Double lines suspected. | |||||||
| HR 787 | BD+52 616 | 16735 | 23556 | 2059 | 02 42 59.7 | +53 31 34 | 5.84 | K0II-III | 9.0 | 12.4 | D:Optical. | ||||||
| HR 788 | 12 | BD+39 610 | 16739 | 55793 | 2187 | S | 896 | 02 42 14.9 | +40 11 38 | 4.91 | F9V | 0.3 | 0.1 | D:0.906y, a = 0.057".,DYN:0.046".,SB:331.0d, K 21.4k/s, V0 -21.5k/s, msin3i 0.744, asini 72.3. Speckle interferometer measurements combined with,SB:spectroscopic yield masses 1.28 and 1.05 solar. Speckle interferometric sep. 0.047", 1981.68. | |||
| HR 792 | BD+47 683 | 16780 | 38274 | 2064 | 02 43 01.9 | +48 15 56 | 6.48 R | G5II | 5.0 | 72.8 | D:AB fixed.,G:UMa stream. | ||||||
| HR 799 | θ | 13 | BD+48 746 | 16895 | 38288 | 93 | I | 2081 | 902 | 02 44 12.0 | +49 13 42 | 4.12 | F8V | 5.6 | 19.6 | D:AB 4.13 F7V, 9.87 M1V, 2720y, a = 22.289". C probably optical.,DYN:0.095". | |
| HR 800 | 14 | BD+43 566 | 16901 | 38289 | 1077 | 02 44 05.2 | +44 17 49 | 5.43 | G0Ib-IICa1CH-1 | ||||||||
| HR 819 | BD+35 553 | 17228 | 55868 | 02 46 58.3 | +35 59 01 | 6.25 | G8III | G:Probable Hyades group. | |||||||||
| HR 820 | BD+34 513 | 17240 | 55872 | 2117 | 02 47 03.5 | +35 33 18 | 6.30 R | A9V | 2.1 | 1.5 | D:AB binary. | ||||||
| HR 825 | BD+56 718 | 17378 | 23637 | S | V480 Per | 02 49 30.8 | +57 05 03 | 6.25 | A5Ia | G:Per OB1; vicinity of Perseus double cluster.,VAR:Amp. 0.038V. | |||||||
| HR 831 | BD+36 566 | 17484 | 55910 | 02 49 27.1 | +37 19 34 | 6.45 | F6III-IV | ||||||||||
| HR 834 | η | 15 | BD+55 714 | 17506 | 23655 | 99 | I | 2157 | 02 50 41.8 | +55 53 44 | 3.76 | K3-Ib-IIa e | 4.7 | 28.3 | C:Large infrared excess.,D:Component B, B9V, CPM, vsini 149k/s.,G:Red star Pleiades group.,N:Miram in Becvar; Allen says unnamed.,S:Ultraviolet FeII emission. Also classified K3Ib. | ||
| HR 840 | 16 | BD+37 646 | 17584 | 55928 | 2194 | W | 956 | 02 50 35.1 | +38 19 07 | 4.23 | F2III | 4.7 | 249.3 | VAR:Delta Sct? | |||
| HR 842 | BD+46 648 | 17656 | 38397 | 2197 | 02 51 41.7 | +46 50 31 | 5.88 | G8III | |||||||||
| HR 843 | 17 | BD+34 527 | 17709 | 55946 | 2198 | I | A | 963 | 02 51 30.8 | +35 03 35 | 4.53 | K5+III | S:Also classified K7III. | ||||
| HR 846 | BD+52 640 | 17743 | 23674 | 2185 | 971 | 02 52 52.0 | +52 59 52 | 6.36 | B8III | 0.2 | 1.6 | D:AB, 7.2, 9.2v sep. 0.2" possibly optical; AC binary.,DYN:0.006". | |||||
| HR 849 | BD+47 723 | 17818 | 38418 | 2192 | 02 53 21.2 | +48 34 10 | 6.26 | G5I | 5.7 | 6.7 | |||||||
| HR 854 | τ | 18 | BD+52 641 | 17878 | 23685 | 103 | I | 2202 | Tau Per | 02 54 15.5 | +52 45 45 | 3.95 | G4III+A4V | 8.6 | 51.7 | D:A* 4.06 G4III+A4V, 4.150y, a = 0.050". Speckle interferometric sep. 0.080" 1981.67. Circumstellar material surrounding,D:the pair? Visual companions 10.7v at 51" possibly physical; 11.8v at 4" possibly optical.,SB:ADS 2202A, 1515.6d, K 19.0k/s, V0 +2.2k/s, asini 271. vsini of secondary 50k/s.,VAR:EA, 3.94 - 4.07V. | |
| HR 855 | 20 | BD+37 655 | 17904 | 55975 | 2200 | 977 | 02 53 42.6 | +38 20 15 | 5.33 | F4IV | 0.6 | 0.2 | D:AB 5.9 F4V, 6.5 F6V, 31.37y, a = 0.258". Nearly equal components, 3.7, 4.3 solar. Component C, 9.7v at 14", CPM?,DYN:0.013".,SB:ADS 2200A, 1269d, K 4.8k/s, V0 +2.4k/s, asini 73.0. Orbit questioned by Morbey and Griffin (1987, ApJ, 317,,SB:343). Resolved by speckle interferometry 1983.93, sep. 0.20"; 1983.94, sep. 0.18".,VAR:Delta Sct? | ||||
| HR 864 | BD+50 665 | 18153 | 23721 | 02 56 50.6 | +51 15 39 | 6.22 | K5III | ||||||||||
| HR 865 | BD+46 658 | 18155 | 38455 | W | 02 56 33.4 | +47 09 50 | 6.02 | gK3 | 5.5 | 24.9 | D:Component B, 15v, possibly spurious. | ||||||
| HR 873 | 21 | BD+31 509 | 18296 | 56031 | 2205 | LT Per | 02 57 17.3 | +31 56 03 | 5.11 | B9pSi v | G:Member moving cluster in Perseus.,S:Underabundance of magnesium and oxygen.,SB:2.88d.,VAR:Alpha CV 5.03 - 5.14V, 2.88422d, same for RV and line-intensities. Also var. magnetic field and H-lines. Rotating,VAR:spotted star. | ||||||
| HR 876 | BD+38 599 | 18339 | 56036 | I | 02 58 02.3 | +38 36 54 | 6.04 | gK3 | |||||||||
| HR 879 | π | 22 | BD+39 681 | 18411 | 56047 | 2207 | 02 58 45.7 | +39 39 46 | 4.70 | A2Vn | N:Gorgonea Secunda. | ||||||
| HR 882 | 24 | BD+34 550 | 18449 | 56052 | 1082 | I | 02 59 03.7 | +35 10 59 | 4.93 | K2III | |||||||
| HR 885 | BD+46 669 | 18474 | 38493 | 02 59 49.9 | +47 13 15 | 5.47 | G5:III* | S:G5:III: CN-4 CH-1 Ca 1 H delta-1. Also classified G8III CH weak. Noted as having composite spectrum, but unresolved,S:by speckle interferometry 1981.69. | |||||||||
| HR 886 | BD+40 639 | 18482 | 38492 | I | 1004 | 02 59 39.9 | +41 01 59 | 5.89 | K2 | ||||||||
| HR 890 | BD+51 665 | 18537 | 23763 | 2270 A | 03 00 52.2 | +52 21 06 | 5.28 | B7V | 1.4 | 11.9 | D:CPM with HR 891.,G:Per OB3. | ||||||
| HR 891 | BD+51 665 | 18538 | 23765 | 2270 B | 03 00 53.4 | +52 21 08 | 6.74 | B9V | 1.4 | 11.9 | D:CPM with HR 890.,G:Per OB1? | ||||||
| HR 894 | BD+37 675 | 18552 | 56067 | 03 00 11.8 | +38 07 54 | 6.11 | B8Vne | S:Shell star. Near IR spectroscopy indicates presence of cool companion. | |||||||||
| HR 915 | γ | 23 | BD+52 654 | 18925 | 23789 | 108 | I | 2324 | 03 04 47.8 | +53 30 23 | 2.93 | G8III+A2V | 8.6 | 57.0 | D:SKYLAB observations indicate cool star with hot companion. Components Aa, 14.65y, a = 0.159". Physical nature of B,,D:11m at 57", uncertain.,M:Close to error box of X-ray source 3U0305+53.,SB:5350d, K 12.7 or 21.9k/s, V0 +2.5k/s, msin3i 4.87, asini 648. vsini of secondary 50k/s. Resolved by speckle,SB:interferometry 1981.67, sep. 0.284", 1983.93, sep. 0.27". | ||
| HR 918 | BD+56 767 | 18970 | 23791 | 2217 | I | 03 05 32.4 | +56 42 21 | 4.76 | G9.5III | ||||||||
| HR 920 | BD+55 738 | 18991 | 23793 | 03 05 39.9 | +56 04 07 | 6.11 | G9III | ||||||||||
| HR 921 | ρ | 25 | BD+38 630 | 19058 | 56138 | 109 | I | Rho Per | 03 05 10.6 | +38 50 25 | 3.39 | M4II | G:Zeta Her group.,N:Gorgonea Tertia.,VAR:SRb 3.30 - 4.0V, about 50d with possibly slow var. in mean brightness in 1100d period. | ||||
| HR 923 | BD+40 664 | 19066 | 38559 | 03 05 20.8 | +40 34 57 | 6.05 | K0III | ||||||||||
| HR 930 | BD+51 681 | 19268 | 23825 | 03 08 03.9 | +52 12 48 | 6.31 | B5V | ||||||||||
| HR 933 | BD+46 692 | 19279 | 38587 | 03 07 47.4 | +47 18 30 | 6.41 | A3Vnn | ||||||||||
| HR 936 | β | 26 | BD+40 673 | 19356 | 38592 | 111 | I | 2362 | Bet Per | 03 08 10.1 | +40 57 20 | 2.12 | B8V | 8.3 | 81.9 | C:Color excess E(B-V) = +0.03.,D:A* var. B8V, 1.858y, a = 0.011" or 1.862y, a = 0.104". Apparent apsidal period 28.4y or 32y. Resolved by speckle,D:interferometry: sep. 0.086", 2-3v fainter than primary. This may be Algol C. Four visual companions all optical:,D:B, 12.7v at 59"; C, 12.5 at 67"; D, 10.5 at 82"; BC sep. 15"; E, 12.5v at 11" from D.,M:One of the few known galactic radio sources in which the dominant star is normal. 21cm radio source.,N:ALGOL; Gorgona; Gorgonea Prima; Demon Star; El Ghoul.,S:B8V+G.,SB:Algol ABxC: 1.8613y, K 12.0k/s, V0 +3.7k/s, msin3i 3.91, asini 109. Spectra B8V, G5IV, Am. Mass Algol AB, 5.3,SB:Suns; C, 1.8 Suns. Circumstellar gas fills Roche lobe of hot component. ADS 19356A: 2.8673d, K 44.0k/s, V0 var.,,SB:asini 1.73. Resolved by speckle interferometry 1982.17, sep. 0.052", 1983.94, sep. 0.08".,VAR:ADS 2362A is the prototype Algol star, first discovered as variable by Montanari in 1669. The first period determined by,VAR:Goodricke in 1783, who also interpreted the variations as due to eclipses. The prototype star proves to be a more,VAR:a complicated system than most of the Algol-type stars, i.e., compact triple system with separation of the components,VAR:well under 0.1". The components usually designated Algol A, B, C, sometimes A, a, P. Two formerly additionally desig-,VAR:nated components D and E, inferred on the basis of an apparent 32 year apsidal motion, are now considered spurious.,VAR:The various Algol components must not be confused with the visual components ADS 2362 B-E, optical companions at much,VAR:greater distances from A. ADS 2362A, EA 2.12 - 3.40V, 2.86732442d, abrupt period changes. Orbital and rotation periods,VAR:synchronized. Rotational velocity 65k/s. Radio flares extending to about 1 A.U., not associated with X-ray activity.,VAR:Radio flare activity appears correlated with period discontinuities, attributed to "starquakes." Mass flow from K to B8,VAR:component at rate of 1.8x10E-08 solar masses/year. Possible circumstellar material associated with radio or H alpha,VAR:emission. | |
| HR 937 | ι | BD+49 857 | 19373 | 38597 | 112 | I | W | 03 09 04.0 | +49 36 48 | 4.05 | G0V | 8.2 | 146.2 | G:Mel 20 #44, but not cluster member; Per OB3. | |||
| HR 941 | κ | 27 | BD+44 631 | 19476 | 38609 | I | 2368 | 1055 | 03 09 29.8 | +44 51 26 | 3.80 | K0III | 8.4 | 27.7 | D:Companion optical.,G:Hyades group. | ||
| HR 947 | ω | 28 | BD+39 724 | 19656 | 56224 | I | W | 03 11 17.4 | +39 36 42 | 4.63 | K1III | 6.1 | 177.4 | N:Gorgonea Quarta. | |||
| HR 949 | BD+47 779 | 19735 | 38638 | 2225 | I | W | 03 12 26.4 | +47 43 33 | 6.33 | K5III | 3.9 | 202.1 | G:Mel 20 #138; Per OB3. | ||||
| HR 950 | BD+41 631 | 19736 | 38635 | 03 12 09.6 | +42 22 34 | 6.15 | B4V | G:Member of the local association (Pleiades group). | |||||||||
| HR 956 | BD+47 782 | 19845 | 38652 | 03 13 24.0 | +48 10 37 | 5.90 | G9III | G:Mel 20 #175; Per OB3. Nonmember of Alpha Per cluster on basis of RV.,M:Space motion same as for Hyades cluster. | |||||||||
| HR 964 | BD+56 798 | 20041 | 23903 | 2424 | 03 15 48.0 | +57 08 27 | 5.79 | A0Ia | 8.2 | 10.8 | G:In reflection nebula; member assoc. Cam R1 at about 870 pc. Cam OB1. | ||||||
| HR 966 | BD+41 638 | 20063 | 38674 | 03 14 56.7 | +42 30 14 | 6.07 R | K2III | S:Strong CN. | |||||||||
| HR 969 | BD+50 729 | 20123 | 23914 | I | 03 16 12.2 | +50 56 16 | 5.03 | G6Ib-IIa | G:Mel 20 #308; Per OB3.,SB:5.543491d. | ||||||||
| HR 973 | BD+44 648 | 20162 | 38685 | I | 03 16 04.7 | +45 20 45 | 6.16 | M2III | |||||||||
| HR 975 | BD+32 591 | 20193 | 56293 | 2431 | 03 15 47.0 | +32 51 23 | 6.31 | F4V vw | 6.5 | 44.1 | |||||||
| HR 976 | BD+34 610 | 20210 | 56296 | 2433 | V423 Per | 03 16 01.9 | +34 41 19 | 6.25 | A1m | 7.2 | 29.3 | SB:ADS 2433A, 5.5435d, K 62.7k/s, V0 +24.2k/s, asini 4.78.,VAR:Ell 6.16 - 6.28V, 5.543491d. | |||||
| HR 978 | BD+31 576 | 20277 | 56308 | 03 16 35.1 | +32 11 01 | 6.06 | G8IV | ||||||||||
| HR 979 | BD+39 743 | 20283 | 38700 | 2443 | 03 17 11.4 | +40 29 00 | 6.45 | B9VpSi | 0.9 | 3.8 | D:Component B, 8.0 A7m. CPM. | ||||||
| HR 982 | 30 | BD+43 674 | 20315 | 38704 | 03 17 47.4 | +44 01 30 | 5.47 | B8V | G:Per OB3; nonmember of Alpha Per cluster on basis of RV. | ||||||||
| HR 986 | BD+38 690 | 20346 | 56322 | 2230 | 03 17 45.8 | +39 17 00 | 5.96 | A2IV | |||||||||
| HR 987 | 29 | BD+49 899 | 20365 | 23944 | 03 18 37.8 | +50 13 20 | 5.15 | B3V | G:Per OB3.,SB:1.996933d. | ||||||||
| HR 989 | 31 | BD+49 902 | 20418 | 38714 | 03 19 07.6 | +50 05 42 | 5.03 | B5V | G:Per OB3. | ||||||||
| HR 991 | BD+33 619 | 20468 | 56340 | 2232 | I | 03 18 43.8 | +34 13 22 | 4.82 | K2IICN1 | S:Also classified K2III CN2 Ba 0.3. | |||||||
| HR 1001 | BD+48 893 | 20675 | 38753 | W | 03 21 52.6 | +49 04 15 | 5.93 | F6V | 3.5 | 205.8 | G:Hyades moving group; Per OB3; Mel 20 #497. | ||||||
| HR 1002 | 32 | BD+42 750 | 20677 | 38750 | 2236 | 1107 | 03 21 26.5 | +43 19 46 | 4.95 | A3V | |||||||
| HR 1011 | BD+48 899 | 20809 | 38768 | 03 23 13.2 | +49 12 48 | 5.29 | B5V | G:Mel 20 #557; Per OB3; nebulosity.,SB:Possibly long period. | |||||||||
| HR 1017 | α | 33 | BD+49 917 | 20902 | 38787 | 120 | I | W | 1125 | 03 24 19.4 | +49 51 40 | 1.79 | F5Ib | 10.0 | 167.0 | G:Mel 20 #605; Per OB3; nebulosity.,N:MIRPHAK; Mirfak; Marfak; Algenib. | |
| HR 1019 | BD+33 636 | 20995 | 56419 | 2514 | 03 24 29.7 | +33 32 09 | 5.61 R | A0V | 3.5 | 4.3 | D:AB CPM. | ||||||
| HR 1020 | BD+53 657 | 21004 | 24024 | 03 25 48.4 | +53 55 18 | 6.51 | A9III-IV | ||||||||||
| HR 1026 | BD+40 736 | 21038 | 38809 | 03 25 09.4 | +41 15 26 | 6.51 | A0V | ||||||||||
| HR 1029 | BD+48 913 | 21071 | 38817 | 03 25 57.4 | +49 07 15 | 6.09 | B7V | G:Mel 20 #675; Per OB3. | |||||||||
| HR 1034 | BD+48 920 | 21278 | 38849 | 03 28 03.1 | +49 03 46 | 4.98 | B5V | C:Color excess E(B-V) = +0.10.,G:Mel 20 #774; Per OB3.,S:Lyman alpha observed from COPERNICUS.,SB:21.659d, K 25.0, V0 -0.5, asini 7.34. | |||||||||
| HR 1037 | BD+49 944 | 21362 | 38862 | 03 28 52.4 | +49 50 54 | 5.58 | B6Vn | G:Mel 20 #810; Per OB3. | |||||||||
| HR 1041 | BD+33 656 | 21402 | 56475 | 03 28 20.8 | +33 48 27 | 5.61 R | A2V | ||||||||||
| HR 1044 | 34 | BD+49 945 | 21428 | 38872 | 2558 | 03 29 22.1 | +49 30 32 | 4.67 | B3V | 2.1 | 0.8 | D:550y.,G:Mel 20 #835; Per OB3. | |||||
| HR 1047 | BD+46 760 | 21455 | 38874 | 2560 | 03 29 26.2 | +46 56 16 | 6.24 | B7V | 5.1 | 27.9 | G:Mel 20 #861; Per OB3. Nonmember of Alpha Per cluster on basis of RV. | ||||||
| HR 1051 | BD+47 844 | 21551 | 38893 | 03 30 37.0 | +48 06 13 | 5.82 | B8V | G:Mel 20 #904; Per OB3.,S:Shell star. | |||||||||
| HR 1052 | σ | 35 | BD+47 843 | 21552 | 38890 | 124 | I | 1167 | 03 30 34.5 | +47 59 43 | 4.36 | K3III | G:Mel 20 #900; Per OB3. | ||||
| HR 1056 | BD+48 938 | 21620 | 38906 | 1173 | 03 31 29.4 | +49 12 35 | 6.29 | A0Vn | G:Mel 20 #934; Per OB3.,VAR:EA, amp. 0.1V, 5.363d. | ||||||||
| HR 1059 | BD+48 942 | 21661 | 38912 | 03 31 49.1 | +49 24 03 | 6.39 | B9III | G:Mel 20 #954; Per OB3. | |||||||||
| HR 1063 | BD+47 847 | 21699 | 38917 | V396 Per | 03 32 08.6 | +48 01 25 | 5.47 | B8IIIpMn | G:Mel 20 #985; Per OB3.,S:Spectra show Mn. Helium weak. Si enhanced. Also classified B5Vp.,VAR:Alpha CV 5.45 - 5.53V, 2.4928d. First helium-weak star found to have periodic variations (1973). | ||||||||
| HR 1069 | 36 | BD+45 778 | 21770 | 38924 | 2249 | 1182 | 03 32 26.3 | +46 03 25 | 5.31 | F4III | |||||||
| HR 1072 | BD+44 734 | 21803 | 38927 | KP Per | 03 32 39.1 | +44 51 20 | 6.41 | B2IV | G:Cas-Tau OB1.,VAR:Beta C 6.37 - 6.47V, 0.2101753d, multiple periods, 0.1982, 10.85, 0.01d. | ||||||||
| HR 1074 | BD+34 674 | 21856 | 56531 | 1098 | Var? | 03 32 40.0 | +35 27 42 | 5.90 | B1V | G:Per OB2. | |||||||
| HR 1078 | BD+39 811 | 21912 | 56538 | 2254 | IW Per | 03 33 35.1 | +39 53 58 | 5.81 | A5m | SB:0.9171877d, K 99.3k/s, V0 +0.2k/s, asini 1.251.,VAR:Ell 5.80 - 5.85V, 0.9171877d. | |||||||
| HR 1087 | ψ | 37 | BD+47 857 | 22192 | 38980 | I | Psi Per | 03 36 29.4 | +48 11 34 | 4.23 | B5Ve v | G:Mel 20 #1164; Per OB3; member of Pleiades group. Nonmember of Alpha Per cluster on basis of RV.,RV:Rotationally unstable shell star.,S:Shell star.,VAR:Amp. 0.04V, 0.5d. Hydrogen emission variable. Expanding circumstellar shell. | |||||
| HR 1097 | BD+42 795 | 22402 | 38999 | 03 38 00.2 | +42 34 59 | 6.42 | B8Vn | ||||||||||
| HR 1113 | BD+37 811 | 22780 | 56628 | 1225 | 03 41 07.9 | +37 34 48 | 5.57 | B7Vne | G:Member of the local association (Pleiades group).,VAR:Gamma Cas?, 5.55 - 5.58V. | ||||||||
| HR 1122 | δ | 39 | BD+47 876 | 22928 | 39053 | 131 | W | Del Per | 03 42 55.5 | +47 47 15 | 3.01 | B5IIIe t | 7.3 | 99.1 | C:Color excess E(B-V) = +0.04.,G:Per OB3.,S:C1 neutral carbon continuum shows discontinuities in UV. Lyman alpha observed from COPERNICUS.,VAR:Alpha CV? 2.98 - 3.03V, about 1d. Strong variable emission at 1650A, CaII? | ||
| HR 1123 | 40 | BD+33 698 | 22951 | 56646 | 2699 | 03 42 22.5 | +33 57 54 | 4.97 | B0.5V | 5.0 | 20.0 | C:Reddened star. Color excess E(B-V) = +0.24.,G:Per OB2. | |||||
| HR 1127 | BD+48 984 | 23049 | 39063 | I | 2712 | 03 44 06.4 | +48 31 25 | 6.06 | K4III | 7.1 | 18.6 | C:Nicolet has 6.60V, Mermilliod 6.39V: no indication of variability. | |||||
| HR 1130 | BD+45 804 | 23139 | 39071 | 2266 | 03 44 40.9 | +46 05 59 | 6.11 | A7IV | |||||||||
| HR 1131 | ο | 38 | BD+31 642 | 23180 | 56673 | 2726 | Omi Per | 03 44 19.1 | +32 17 18 | 3.83 | B1III | 2.8 | 1.0 | C:Reddened star. Color excess E(B-V) = +0.32.,D:Binary. Combined mag., colors. Rotational velocity B, 150:k/s. Unresolved by speckle interferometry 1982.16.,DYN:0.005".,G:Per OB2 (not a member). Embedded in reflection nebulosity. In cluster IC 348.,M:In interstellar ultraviolet radiation field.,N:Atik; Ati; Al Atik.,P:Intrinsic polarization, probably due to circumstellar matter.,SB:4.4192d, K 109.3k/s, V0 +19.8k/s, msin3i 5.26, asini 6.63. Rotational velocity of secondary, 84k/s, primary,SB:85k/s.,VAR:Ell 3.79 - 3.85V, 4.419171d, possibly half. | |||
| HR 1133 | BD+36 742 | 23193 | 56675 | 2268 | 03 44 31.4 | +36 27 36 | 5.59 | A2m | |||||||||
| HR 1135 | ν | 41 | BD+42 815 | 23230 | 39078 | 134 | I | 2738 | 1261 | 03 45 11.6 | +42 34 43 | 3.77 | F5II | 8.1 | 31.4 | ||
| HR 1141 | BD+45 811 | 23300 | 39085 | 2746 | 03 45 59.3 | +45 40 55 | 5.66 | B6V | 8.4 | 6.5 | D:CPM.,G:Member of the local association (Pleiades group). | ||||||
| HR 1160 | BD+50 825 | 23552 | 24231 | 2769 | 03 48 18.3 | +50 44 12 | 6.14 | B8Vne | 6.2 | 7.0 | D:Probably optical.,S:Shell star. | ||||||
| HR 1163 | BD+33 717 | 23625 | 56709 | 2772 | 1305 | 03 47 52.6 | +33 36 00 | 6.57 | B2.5V | 4.0 | 3.2 | D:Binary.,G:Per OB2.,SB:ADS 2772A, 1.9406d, K 82k/s, V0 +20k/s, msin3i 0.883, asini 2.19.,VAR:B-A varies from 2.8 to 4.3V. Uncertain which component varies. | |||||
| HR 1164 | BD+31 650 | 23626 | 56707 | 03 47 48.9 | +32 11 42 | 6.25 | G0 | ||||||||||
| HR 1170 | BD+43 818 | 23728 | 39128 | V376 Per | 03 49 08.2 | +43 57 47 | 6.02 | A9IV | VAR:Delta Sct 5.8 - 5.91V, variable amp. Primary and beat periods, 0.098299 and 0.39206d. | ||||||||
| HR 1176 | BD+44 801 | 23838 | 39134 | Var? | 03 50 04.5 | +44 58 04 | 5.66 | G2III+F2:V | SB:vsini of secondary 85k/s. Unresolved by speckle interferometry 1983.93.,VAR:A variable comparison star was used when HR 1176 was suspected of variablility. | ||||||||
| HR 1177 | 42 | BD+32 667 | 23848 | 56727 | V467 Per | 03 49 32.6 | +33 05 29 | 5.11 | A3V | G:Per OB2.,SB:1.7653d, K 34.4k/s, V0 -11.9k/s, asini 0.832.,VAR:A published period, 22.58d, does not satisfy available SB observations, whereas the SB period does satisfy the,VAR:photometric equally well. However, more observations are badly needed. | |||||||
| HR 1191 | BD+33 728 | 24131 | 56761 | W | 03 51 53.7 | +34 21 33 | 5.77 | B1V | 7.5 | 15.1 | G:Per OB2. | ||||||
| HR 1197 | BD+30 582 | 24167 | 56762 | 03 52 04.3 | +31 10 06 | 6.25 | A5V | G:Per OB2. | |||||||||
| HR 1198 | BD+48 1015 | 24240 | 39175 | 03 53 38.7 | +48 39 02 | 5.76 | K0III | ||||||||||
| HR 1203 | ζ | 44 | BD+31 666 | 24398 | 56799 | 144 | I | 2843 | 1397 | 03 54 07.9 | +31 53 01 | 2.85 | B1Ib | 6.5 | 12.9 | C:Reddened star. Color excess E(B-V) = +0.33.,D:AB CPM, B 9.16V B8IV; C, 9.12V at 33" optical; D, 10.35V, +0.713(B-V), +0.20(U-B), at 92" optical; E, 9.90V, A2V,,D:+0.33(B-V), +0.17(U-B), at 120" physical.,DYN:0.012".,G:IC 348; Per OB2.,RV:Comp. B +20.8k/s.,S:Interstellar CH detected optically. COPERNICUS data used to analyze the chemical abundances in line of sight to,S:Zeta Per: CO, HD, and OH. About 60% of the hydrogen in front of the star is molecular.,SB:1.765d, K 6.0k/s, V0 +22.2k/s.,VAR:2.80 - 2.93V. | |
| HR 1207 | BD+47 912 | 24504 | 39195 | 2279 | 03 55 58.2 | +47 52 17 | 5.37 | B6V | G:Per OB3. | ||||||||
| HR 1209 | BD+30 591 | 24534 | 56815 | I | 2859 | X Per | 03 55 23.0 | +31 02 45 | 6.10 | O9.5ep v | 5.8 | 22.5 | C:Heavily reddened.,D:CPM? Component A possibly optical counterpart or companion of X-ray source 4U0352+30. Possibly a triple system with a,D:neutron star moving around the optical primary in 22.4 hrs., and either apsidal period 581d or close double moving,D:around a distant component in 581d. Rotational velocity of primary, vsini 306k/s. Component ADS 2859B is normal M1III,,D:not T Tau type as once assumed.,G:May not be member of Per OB2; Zeta Per group.,M:Space velocities of X Per and Xi Per indicate the two stars approached to within 17 pc 2 million yrs ago.,P:Conflicting evidence whether observed polarization is intrinsic to the star or of interstellar origin.,S:Sp. data suggest occasional interruption of almost steady infall of material through rotating emission region by,S:outbursts of material from the star.,SB:580.7d, K 59k/s, V0 -50k/s, asini 471. Emission lines var. in RV, 22.4 hrs. and 581d.,VAR:ADS 2859A, Gamma Cas 6.07 - 7.0V, 580.7?d. Amp. about 0.02U. X-ray period 22.4 hrs. Spectrum variable. Sudden,VAR:decrease in H alpha emission followed by 450 sec. flare in continuum. Possible neutron star companion pulsating in,VAR:13.924 min. Simultaneous X-ray and optical obs. 21 Jan. 1975 showed X-ray var. by factor 2 but no corresponding optical,VAR:100 sec. quasi periodic photometric var. may indicate binary with compact companion undergoing mass accretion. | ||||
| HR 1210 | 43 | BD+50 860 | 24546 | 24314 | I | W | 03 56 36.5 | +50 41 43 | 5.28 | F5IV | 4.8 | 75.3 | C:IR source in this direction corresponds to a Seyfert galaxy.,D:AB CPM. Component C, 11.4v at 101" optical. P, 12.5v at 279".,G:Hyades moving group.,SB:30.4380d, K 51.9k/s, V0 +25.1k/s, msin3i 0.910, asini 16.9; alternate orbit 30.4391d, K50.6k/s,,SB:msin3i 0.82, asini 15.53; vsini both components <17k/s. | ||||
| HR 1215 | BD+34 768 | 24640 | 56824 | 1418 | 03 56 28.7 | +35 04 52 | 5.49 | B1.5V | G:Per OB2.,VAR:Beta C?, 5.45 - 5.50V. RV possibly var. 0.13169d. | ||||||||
| HR 1220 | ε | 45 | BD+39 895 | 24760 | 56840 | 147 | 2888 | Eps Per | 03 57 51.2 | +40 00 37 | 2.89 | B0.5V+A2V | 5.1 | 8.8 | C:Color excess E(B-V) = +0.10.,D:AB CPM. B, 7.39V, -0.03(B-V), -0.52(U-B), B9.5V, vsini 300:k/s.,G:Cas-Tau OB1; member of Pleiades group.,VAR:Beta C, 2.88 - 3.00V, 0.216:d. Brightest component on visual triple. Photoelectric and spectroscopic resonant periods,VAR:found are submultiples of 26.9 hrs or 1.12d. | ||
| HR 1223 | BD+34 773 | 24809 | 56847 | V386 Per | 03 58 03.1 | +34 48 52 | 6.53 | A8V | G:Per OB2.,SB:vsini both components 80k/s.,VAR:Delta Sct 6.50 - 6.58V, 0.052d. | ||||||||
| HR 1226 | BD+38 827 | 24843 | 56849 | 03 58 29.1 | +38 50 25 | 6.30 | gK1 | ||||||||||
| HR 1228 | ξ | 46 | BD+35 775 | 24912 | 56856 | 148 | I | Xi Per | 03 58 57.9 | +35 47 28 | 4.04 | O7.5III(n)((f)) e | C:Color excess E(B-V) = +0.32.,G:Runaway star from Per OB2. Within 1d and exciting star of HII region S220. Ionizes region at edge of California nebula =,G:NGC 1499.,N:Menkib; Menkhib; Menchib.,S:Interstellar CO emission. Central Balmer emission in blue-violet only.,SB:6.951d.,VAR:Slightly variable, possibly same period as SB. | ||||
| HR 1229 | BD+38 829 | 24982 | 56866 | 2910 | 03 59 40.0 | +38 49 14 | 6.38 R | A1Vp: | 2.7 | 1.5 | |||||||
| HR 1234 | BD+36 805 | 25152 | 56899 | 04 01 14.7 | +36 59 24 | 6.41 | A0V | RV:Determinations of vsini range from 50 to 250k/s. | |||||||||
| HR 1261 | λ | 47 | BD+49 1101 | 25642 | 24412 | 1113 | 04 06 35.0 | +50 21 05 | 4.29 | A0IVn | |||||||
| HR 1273 | 48 | BD+47 939 | 25940 | 39336 | 152 | I | MX Per | 04 08 39.7 | +47 42 45 | 4.04 | B3Ve | G:Per OB3; member of Pleiades group.,RV:Pole on.,S:Excess IR emission.,SB:16.934615d not confirmed.,VAR:Gamma Cas 4.00 - 4.10V, 55?d. Slow var. possibly associated with emission spectrum. | |||||
| HR 1277 | 49 | BD+37 881 | 25975 | 57000 | 04 08 15.3 | +37 43 40 | 6.09 | K1III | |||||||||
| HR 1278 | 50 | BD+37 882 | 25998 | 57006 | 2297 | 04 08 36.6 | +38 02 23 | 5.51 | F7V | D:CPM with GC 4949 at 12' = ADS 2995, a triple system 7.3 dK2, 9.0 sep. 1"; C at 234".,G:Hyades group. | |||||||
| HR 1286 | BD+33 807 | 26311 | 57047 | 2300 | I | 04 10 59.0 | +33 35 12 | 5.72 | K1II-III | ||||||||
| HR 1301 | BD+37 897 | 26605 | 57081 | 04 13 59.6 | +37 58 01 | 6.45 R | G9III | ||||||||||
| HR 1303 | μ | 51 | BD+48 1063 | 26630 | 39404 | 1117 | I | 3071 | 1518 | 04 14 53.9 | +48 24 34 | 4.14 | G0Ib | 6.0 | 83.8 | D:A* 4.13 G0Ib, 0.778y, a = 0.019". AB CPM; B, 11.8v at 15". C , 10.25V, +0.47(B-V), +0.06(U-B), B8.,SB:283.272d, K 20.7k/s, V0 +7.7k/s, asini 80.5. Unresolved by speckle interferometry.,VAR:ADS 3071A, 4.1 - 4.24V. | |
| HR 1306 | 52 | BD+40 912 | 26673 | 39409 | 2306 | I | 04 14 53.3 | +40 29 01 | 4.71 | G5Ib+A2V | SB:1576.44d, K 18.1k/s, V0 -4.5k/s, asini 358. Unresolved by speckle interferometry 1983.93. vsini of secondary,SB:100k/s. | ||||||
| HR 1324 | BD+49 1150 | 26961 | 24531 | b Per | 04 18 14.6 | +50 17 44 | 4.61 | A2V | G:In NGC 1545 #1; Hyades group.,M:Source of weak radio emission.,SB:Comp. ABC: 701.76d, K 11.4k/s, V0 +21k/s, asini 107. Comp. A: 1.527365d, K 39.4k/s, V0 var., asini 0.827.,SB:Unresolved by speckle interferometry.,VAR:Ell 4.59 - 4.65V, 1.527365d. Radio binary showing radio flare activity. Third component may eclipse primary. | ||||||||
| HR 1328 | BD+41 844 | 27026 | 39447 | 04 18 08.2 | +42 08 28 | 6.22 | B9V | ||||||||||
| HR 1330 | BD+49 1155 | 27084 | 39457 | 04 19 13.3 | +50 02 56 | 5.45 | A7V | G:NGC 1545 #1. | |||||||||
| HR 1333 | BD+50 973 | 27192 | 24544 | 2316 | 1550 | 04 20 11.5 | +50 55 15 | 5.55 | B1.5IV | G:Cas-Tau OB1.,SB:1.527365d, K 38.83k/s, V0 +20.66k/s, asini 0.815.,VAR:Amp. 0.020V. | |||||||
| HR 1337 | BD+41 852 | 27278 | 39468 | 04 20 14.4 | +41 48 29 | 5.92 | K0III | ||||||||||
| HR 1343 | 54 | BD+34 860 | 27348 | 57171 | 158 | I | W | 04 20 24.6 | +34 34 00 | 4.93 | G8III | 7.9 | 110.0 | ||||
| HR 1344 | BD+31 757 | 27349 | 57166 | I | 04 20 10.0 | +31 57 12 | 6.16 | K5 | |||||||||
| HR 1350 | 53 | BD+46 872 | 27396 | 39483 | 2319 | V469 Per | 04 21 33.2 | +46 29 56 | 4.85 | B4IV | G:Member of Pleiades group.,SB:Same period as VAR.,VAR:Amp. 0.01V, 7.29?hrs. | ||||||
| HR 1371 | BD+42 946 | 27650 | 39501 | 3172 | 04 23 35.9 | +42 25 41 | 6.23 | A1pSi | 0.5 | 0.4 | |||||||
| HR 1377 | 55 | BD+33 853 | 27777 | 57212 | 04 24 29.2 | +34 07 50 | 5.73 | B8V | |||||||||
| HR 1379 | 56 | BD+33 854 | 27786 | 57216 | 3188 | 1592 | 04 24 37.4 | +33 57 35 | 5.76 | F4V | 3.6 | 4.9 | DYN:0.042".,VAR:ADS 3188B, 9.6 - 11.3v. | ||||
| HR 1390 | BD+31 776 | 27971 | 57229 | 2325 | 04 26 06.3 | +31 26 20 | 5.28 | K1III | |||||||||
| HR 1419 | BD+32 806 | 28459 | 57269 | W | 04 30 38.3 | +32 27 29 | 6.21 | B9.5Vn | D:Suspected of being double; probably single. | ||||||||
| HR 1424 | BD+39 1013 | 28503 | 57278 | 3273 A | 04 31 24.0 | +40 00 37 | 6.26 | B8V | 0.5 | 9.3 | D:CPM. | ||||||
| HR 1434 | 57 | BD+42 990 | 28704 | 39604 | 1124 | W | 04 33 24.9 | +43 03 50 | 6.09 | F0V | 0.7 | 116.2 | |||||
| HR 1454 | 58 | BD+40 1000 | 29094 | 39639 | 2338 | I | A | 04 36 41.4 | +41 15 53 | 4.25 | K4III+A3V | 0.1 | D:A* 4.27 G8II+B, 28.67y, a = 0.054"(not confirmed).,S:Also classified K0II-III + B9V.,SB:10,470d, K 12.8k/s, V0 +5.9k/s, asini 1400. One of the longest SB periods known, 28.67y. Masses 6 and 5 solar.,SB:Unresolved by speckle interferometry. vsini of both components =<50k/s. | ||||
| HR 1482 | BD+48 1128 | 29526 | 39688 | 2347 | 04 41 24.1 | +48 18 03 | 5.67 | A0V | |||||||||
| HR 1489 | BD+37 954 | 29645 | 57377 | 2348 | 04 41 50.3 | +38 16 49 | 5.99 | G0V | |||||||||
| HR 1493 | BD+49 1230 | 29721 | 39702 | 1128 | W | 04 43 21.6 | +49 58 26 | 5.87 | B9III | 7.3 | 20.8 | ||||||
| HR 1494 | 59 | BD+43 1043 | 29722 | 39699 | 2349 | 04 42 54.3 | +43 21 54 | 5.29 | A1Vn | ||||||||
| HR 1500 | BD+40 1032 | 29866 | 39715 | 04 44 12.9 | +40 47 13 | 6.08 | B8IVne | S:Shell star. | |||||||||
| HR 1514 | BD+40 1045 | 30138 | 39746 | 04 46 44.4 | +40 18 46 | 5.97 | G9III | ||||||||||
| HR 1533 | BD+37 969 | 30504 | 57447 | 1133 | I | 04 49 54.6 | +37 29 18 | 4.88 | K3.5IIIBa0.2: | N:Formerly 1 Aur, now in Perseus. |
| Planetary Nebulae | ||||||||
|---|---|---|---|---|---|---|---|---|
| Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
| NGC 650 | 01 42 18.1 | +51 34 17 | PN | 12.2 | 10.1 | 3.12 | vB, p of D neb | M 76, PK 130-10.1, CS=17.0, Little Dumbbell (SW) |
| IC 351 | 03 47 33.0 | +35 02 50 | PN | 12.4 | 11.9 | 0.3 | Planetary = * 10m, * 9m p 14s, 2' s | PK 159-15.1, CS=15.0 |
| IC 2003 | 03 56 22.0 | +33 52 32 | PN | 12.6 | 11.4 | 0.33 | pB, eS, lE ns, * 13 n 4", * 12 sp 18" | PK 161-14.1, CS=15.3 |
| Galactic Nebulae | ||||||||
| Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
| NGC 1333 | 03 29 18.0 | +31 25 00 | RN | 6 × 3 | F, L, * 10 nf (Auw No 17) | LBN 741 | ||
| NGC 1491 | 04 03 13.5 | +51 18 58 | EN | 25 × 25 | vB, S, iF, bM, r, * inv | LBN 704, in Sh2-206 | ||
| NGC 1499 | 04 01 10.0 | +36 27 36 | EN | 5.0 | 120 × 60 | vF, vL, E ns, dif | LBN 756, California nebula | |
| NGC 1579 | 04 30 14.2 | +35 16 47 | RN | 12 × 8 | pB, vL, iR, mbM, * 8 350°, 2' | LBN 766, Sh2-222 | ||
| IC 2067 | 04 30 52.0 | +35 26 42 | EN | vF, R, * 15 inv n, * 17 close np | SS 20 | |||
| Open Clusters | ||||||||
| Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
| NGC 744 | 01 58 33.0 | +55 28 24 | IV2p | 7.9 | 5 | Cl, pL, pRi, iF, st 11…13 | OCL 345 | |
| NGC 869 | 02 19 04.0 | +57 08 06 | I3r | 5.3 | 18 | ! Cl, vvL, vRi, st 7…14 | OCL 350, Chi Per, Double cluster | |
| NGC 884 | 02 22 05.0 | +57 07 48 | I3r | 6.1 | 18 | ! Cl, vL, vRi, ruby * M | OCL 353, Chi Per, Double cluster | |
| NGC 957 | 02 33 21.0 | +57 33 36 | III2p | 7.6 | 10 | Cl, pL, pRi, st 13…15 | OCL 362 | |
| NGC 1039 | 02 42 05.0 | +42 45 42 | II3m | 5.2 | 25 | Cl, B, vL, lC, sc st 9 | M 34, OCL 382 | |
| NGC 1193 | 03 05 55.0 | +44 23 00 | II3m | 12.6 | 3 | F, cL, er | OCL 390 | |
| NGC 1220 | 03 11 40.6 | +53 20 53 | II2p | 11.8 | 2 | Cl, vS, st vF | OCL 380 | |
| NGC 1245 | 03 14 41.4 | +47 14 19 | III1r | 8.4 | 10 | Cl, pL, Ri, C, iR, st 12…15 | OCL 389 | |
| NGC 1342 | 03 31 38.0 | +37 22 36 | III3p | 6.7 | 17 | Cl, vL, ab 60 st | OCL 401 | |
| NGC 1348 | 03 34 06.0 | +51 25 12 | II2p | 6 | Cl, lRi, st L | OCL 391 | ||
| NGC 1444 | 03 49 25.0 | +52 39 18 | IV1p | 6.6 | 4 | Cl of ab 30 st 12…14 | OCL 394 | |
| NGC 1496 | 04 04 31.8 | +52 39 41 | II1p | 9.6 | 3 | Cl, segment of a ring | OCL 396 | |
| NGC 1513 | 04 09 57.0 | +49 30 54 | II1m | 8.4 | 12 | Cl, L, vRi, pC, st vL | OCL 398 | |
| NGC 1528 | 04 15 19.0 | +51 12 42 | II2m | 6.4 | 18 | Cl, B, vRi, cC | OCL 397 | |
| NGC 1545 | 04 20 56.2 | +50 15 19 | II2p | 6.2 | 12 | Cl, pRi, lC, st L | OCL 399 | |
| NGC 1582 | 04 31 39.0 | +43 44 36 | IV2p | 7.0 | 24 | Cl, vL, pRi, lC, st L | OCL 407 | |
| NGC 1605 | 04 34 52.2 | +45 16 17 | III1m | 10.7 | 5 | Cl, vF, pS, C, st eS | OCL 406 | |
| NGC 1624 | 04 40 36.4 | +50 27 42 | I2pn | 11.8 | 3 | F, cL, iF, 6 or 7 st + neb | OCL 403, LBN 722, Ced 37, S 212 | |
| IC 348 | 03 44 34.1 | +32 09 47 | IV2pn | 7.3 | 10 | pB, vL, vgbM | IC 1985, OCL 409, LBN 758, CED 20 | |
| Galaxies | ||||||||
| Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
| NGC 832 | 03 11 05.4 | +35 23 11 | E2 | 13.9 | 12.9 | 1.6 × 1.3 | F, vS, * 9·10 sp | NGC 1226, UGC 2575, MCG 6-8-1, CGCG 525-2, CGCG 524-61 |
| NGC 1001 | 02 39 12.6 | +41 40 18 | Sbc | 15.6 | 14.8 | 0.7 × 0.3 | vF, vS | MCG 7-6-50, CGCG 539-69 |
| NGC 1003 | 02 39 16.6 | +40 52 22 | Sc | 12.0 | 11.5 | 4.3 × 1.3 | pF, L, E 90° ±, mbM, r | UGC 2137, MCG 7-6-51, CGCG 539-70, IRAS 02360+4039 |
| NGC 1005 | 02 39 27.6 | +41 29 36 | E-S0 | 14.8 | 13.8 | 1 × 0.8 | vF, vS | MCG 7-6-52, CGCG 539-71 |
| NGC 1023 | 02 40 24.1 | +39 03 48 | E/SB0 | 10.4 | 9.4 | 7.4 × 2.5 | vB, vL, vmE, vvmbM | UGC 2154, MCG 6-6-73, CGCG 523-83, Arp 135 |
| NGC 1023 A | 02 40 36.9 | +39 03 37 | IBm | 14.3 | 13.6 | 1.3 × 0.7 | vB, vL, vmE, vvmbM | Arp 135 |
| NGC 1040 1 | 02 43 12.5 | +41 30 01 | S0 | 13.9 | 12.9 | 1.7 × 0.8 | F, S, bM | NGC 1053-1, UGC 2187, MCG 7-6-60, CGCG 539-83 |
| NGC 1040 2 | 02 43 12.1 | +41 30 54 | S0 | 16.3 | 15.3 | 0.4 × 0.2 | F, S, bM | NGC 1053-2, NPM1G +41.0081 |
| NGC 1050 | 02 42 35.6 | +34 45 51 | SBa | 13.5 | 12.6 | 1.7 × 1.1 | F, S, * 18 inv n | UGC 2178, MCG 6-6-78, CGCG 523-92, IRAS 02395+3433, KUG 0239+345, KARA 116, CGCG 524-1 |
| NGC 1058 | 02 43 29.9 | +37 20 29 | Sc | 11.8 | 11.2 | 2.5 × 2.5 | pF, cL, R, glbM | UGC 2193, MCG 6-7-1, CGCG 524-5, IRAS 02403+3707, CGCG 523-96, KUG 0240+371 |
| NGC 1077 A | 02 46 00.6 | +40 05 24 | Sb | 14.4 | 13.6 | 1.1 × 0.8 | vF, pL, E | UGC 2230, MCG 7-6-69, CGCG 539-95, IRAS 02428+3952 |
| NGC 1077 B | 02 46 02.9 | +40 05 36 | SBb | 17.1 | 16.3 | 0.5 × 0.4 | vF, pL, E | MCG 7-6-68, CGCG 539-95 |
| NGC 1086 | 02 47 56.2 | +41 14 48 | Sc | 13.5 | 12.8 | 1.5 × 1 | vF, pS, D * nr | UGC 2258, MCG 7-6-71, CGCG 539-101, IRAS 02447+4102 |
| NGC 1106 | 02 50 40.5 | +41 40 20 | S0 | 13.3 | 12.3 | 1.3 × 1 | vF, vS, vF * att s | UGC 2322, MCG 7-6-76, CGCG 539-112, IRAS 02474+4127 |
| NGC 1123 | 02 52 51.2 | +42 12 19 | SBb | 12.9 | 12.1 | 1.8 × 1.3 | cF, S, iR, vgbM, r | NGC 1122, UGC 2353, MCG 7-6-83, CGCG 539-117, IRAS 02496+4200 |
| NGC 1129 | 02 54 27.3 | +41 34 47 | E3 | 13.5 | 12.4 | 2.9 × 2.1 | cF, pS, iR, vglbM, D or F * sp | UGC 2373, MCG 7-7-4, CGCG 539-124, VV 85, CGCG 540-6 |
| NGC 1130 | 02 54 24.5 | +41 36 22 | C | 16.1 | 15.1 | 0.5 × 0.3 | eF, eS | MCG 7-7-2, CGCG 539-122, CGCG 540-4 |
| NGC 1131 | 02 54 34.0 | +41 33 33 | E0 | 15.6 | 14.6 | 0.4 × 0.4 | eF, eS | MCG 7-7-5, CGCG 539-125, CGCG 540-7, 5ZW 286 |
| NGC 1138 | 02 56 36.3 | +43 02 50 | SB0 | 13.8 | 12.8 | 1.1 × 1.1 | vF, vS, R, gbM, 2 S st Δ | UGC 2408, MCG 7-7-12, CGCG 540-15 |
| NGC 1159 | 03 00 46.4 | +43 09 46 | S0 | 14.5 | 13.5 | 0.5 × 0.4 | vF, S, R, vlbM | UGC 2467, CGCG 540-23, IRAS 02575+4257 |
| NGC 1160 | 03 01 13.2 | +44 57 20 | Scd | 13.5 | 12.8 | 1.5 × 0.7 | F, E | UGC 2475, MCG 7-7-14, CGCG 540-27, KCPG 86A, IRAS 02579+4445 |
| NGC 1161 | 03 01 14.1 | +44 53 51 | S0 | 12.1 | 11.0 | 2.8 × 2 | F, pS, lE, sbM | UGC 2474, MCG 7-7-15, CGCG 540-26, KCPG 86B, IRAS 02579+4442 |
| NGC 1164 | 03 01 59.8 | +42 35 08 | SBab | 13.9 | 13.1 | 1.3 × 1.1 | eF, vS | UGC 2490, MCG 7-7-16, MK 1067, IRAS 02587+4223, CGCG 540-28, NPM1G +42.0105 |
| NGC 1167 | 03 01 42.3 | +35 12 21 | S0 | 13.4 | 12.4 | 3.3 × 2.3 | vF, pL, R, spmbM | UGC 2487, MCG 6-7-33, CGCG 524-45 |
| NGC 1169 | 03 03 34.8 | +46 23 11 | SBb | 12.2 | 11.3 | 4 × 2.6 | pF, pS, iF, sbM | UGC 2503, MCG 8-6-25, CGCG 554-20 |
| NGC 1171 | 03 03 58.9 | +43 23 52 | Sc | 13.0 | 12.3 | 1.9 × 1 | vF, pL, iF | UGC 2510, MCG 7-7-18, CGCG 540-31, IRAS 03006+4312 |
| NGC 1175 | 03 04 32.3 | +42 20 25 | S0-a | 13.9 | 12.9 | 1.9 × 0.7 | F, cL, E | UGC 2515, MCG 7-7-19, CGCG 540-32 |
| NGC 1177 | 03 04 37.2 | +42 21 46 | S | 15.4 | 14.6 | 0.4 × 0.4 | vF, S, R, nf II 607 | IC 281, MCG 7-7-20, CGCG 540-33 |
| NGC 1186 | 03 05 30.9 | +42 50 08 | SBbc | 12.2 | 11.4 | 3.2 × 1.2 | F * with neb appendages | NGC 1174, UGC 2521, MCG 7-7-21, CGCG 540-34, IRAS 03022+4238 |
| NGC 1198 | 03 06 13.3 | +41 50 56 | E-S0 | 13.5 | 12.5 | 1.4 × 0.8 | Neb * 11 | IC 282, UGC 2533, MCG 7-7-24, CGCG 540-38 |
| NGC 1207 | 03 08 15.4 | +38 22 56 | Sb | 13.5 | 12.7 | 2.3 × 1.6 | cF, vS, R, psb in npp end | UGC 2548, MCG 6-7-43, CGCG 524-55, KCPG 87, IRAS 03050+3811 |
| NGC 1212 | 03 09 42.3 | +40 53 35 | S0-a | 15.5 | 14.6 | 1 × 0.5 | eF, S, R, Algol nr | IC 1883, UGC 2560 |
| NGC 1213 | 03 09 17.3 | +38 38 57 | Sd | 15.0 | 14.4 | 1.8 × 1.4 | eF, lE, * close n, diffic | IC 1881, UGC 2557, MCG 6-7-45, CGCG 524-58 |
| NGC 1224 | 03 11 13.5 | +41 21 48 | E-S0 | 15.0 | 14.0 | 1 × 0.8 | eF, vS, R | UGC 2578, MCG 7-7-34, CGCG 540-55 |
| NGC 1227 | 03 11 07.8 | +35 19 31 | SB0-a | 15.1 | 14.2 | 1 × 0.9 | vF, vS | UGC 2577, CGCG 525-3, CGCG 524-62 |
| NGC 1233 | 03 12 33.1 | +39 19 09 | Sb | 14.0 | 13.2 | 1.8 × 0.6 | F, vS, R, diff | NGC 1235, UGC 2586, MCG 6-8-3, IRAS 03093+3907, CGCG 525-6, CGCG 524-65 |
| NGC 1250 | 03 15 21.0 | +41 21 20 | S0 | 14.0 | 12.9 | 2.1 × 0.6 | vF, vS, R | UGC 2613, MCG 7-7-40, CGCG 540-66 |
| NGC 1259 | 03 17 17.3 | +41 23 08 | S0 | 15.3 | 14.3 | 0.7 × 0.7 | vF, S, R, vlbM | MCG 7-7-46 |
| NGC 1260 | 03 17 27.2 | +41 24 19 | S0-a | 14.2 | 13.3 | 1.1 × 0.5 | vF, S, R | UGC 2634, MCG 7-7-47, CGCG 540-81, IRAS 03141+4113 |
| NGC 1264 | 03 17 59.5 | +41 31 13 | SBab | 14.9 | 14.1 | 1 × 0.5 | vF, S, vlbM | UGC 2643, MCG 7-7-50 |
| NGC 1265 | 03 18 08.4 | +41 45 16 | E5 | 14.4 | 13.4 | 1 × 0.5 | vF, vS, mbM | IC 312, UGC 2644, MCG 7-7-51, CGCG 540-86 |
| NGC 1267 | 03 18 44.8 | +41 28 03 | E2 | 14.1 | 13.1 | 1.1 × 0.9 | F, vS, R, stell | UGC 2657, MCG 7-7-55, CGCG 540-92 |
| NGC 1268 | 03 18 45.2 | +41 29 21 | Sb | 14.2 | 13.4 | 0.9 × 0.6 | eF, S, lE, com | UGC 2658, MCG 7-7-56, CGCG 540-93 |
| NGC 1270 | 03 18 58.1 | +41 28 13 | E2 | 14.3 | 13.1 | 0.9 × 0.7 | vF, S, R | UGC 2660, MCG 7-7-57, CGCG 540-95 |
| NGC 1271 | 03 19 11.2 | +41 21 13 | SB0? | 14.9 | 13.9 | 0.5 × 0.2 | vF, vS | CGCG 540-96 |
| NGC 1272 | 03 19 21.3 | +41 29 26 | E1 | 12.9 | 11.8 | 2.2 × 2 | F, S, R | UGC 2662, MCG 7-7-58, CGCG 540-98 |
| NGC 1273 | 03 19 26.8 | +41 32 24 | S0 | 14.3 | 13.2 | 0.8 × 0.7 | vF, vS | MCG 7-7-59, CGCG 540-99 |
| NGC 1274 | 03 19 40.6 | +41 32 58 | E3 | 15.1 | 14.1 | 0.8 × 0.3 | vF, vS | MCG 7-7-62, CGCG 540-102 |
| NGC 1275 | 03 19 48.1 | +41 30 41 | S0/P | 12.6 | 11.9 | 2.3 × 1.6 | F, S | UGC 2669, MCG 7-7-63, CGCG 540-103, 3C 84 , IRAS 03164+4119, Perseus A |
| NGC 1277 | 03 19 51.4 | +41 34 27 | S0-a | 14.7 | 13.6 | 0.8 × 0.3 | vF, vS, np II 603 | MCG 7-7-64, CGCG 540-104 |
| NGC 1278 | 03 19 54.1 | +41 33 49 | E2 | 13.6 | 12.4 | 1.4 × 1.1 | pB, pS, R, bM | IC 1907, UGC 2670, MCG 7-7-65, CGCG 540-105 |
| NGC 1279 | 03 19 59.1 | +41 28 47 | S | 15.8 | 15.0 | 0.6 × 0.4 | vF, vS | PGC 12449 |
| NGC 1281 | 03 20 06.3 | +41 37 47 | E5 | 14.5 | 13.3 | 0.9 × 0.4 | vF, S, * 11 p 1' | MCG 7-7-67, CGCG 540-108 |
| NGC 1282 | 03 20 12.0 | +41 22 01 | E4 | 13.9 | 12.9 | 1.2 × 0.7 | vF, S, lbMN | UGC 2675, MCG 7-7-68, CGCG 540-109 |
| NGC 1283 | 03 20 15.5 | +41 23 55 | E1 | 14.7 | 13.6 | 0.7 × 0.6 | vF, S, vlbM | UGC 2676, MCG 7-7-69, CGCG 540-110 |
| NGC 1293 | 03 21 36.4 | +41 23 36 | E0 | 14.5 | 13.4 | 0.9 × 0.9 | vF, R, bM, np of 2 | MCG 7-7-75, CGCG 540-116, NPM1G +41.0114 |
| NGC 1294 | 03 21 40.0 | +41 21 38 | E-S0 | 14.3 | 13.2 | 1.1 × 0.8 | vF, R, bM, sf of 2 | UGC 2694, MCG 7-7-76, CGCG 540-117, IRAS 03184+4111 |
| NGC 1334 | 03 30 01.7 | +41 49 57 | Sbc | 14.0 | 13.2 | 1.5 × 0.7 | eF, pL, lbM | UGC 2759, MCG 7-8-18, CGCG 541-17, IRAS 03266+4139 |
| NGC 1335 | 03 30 19.4 | +41 34 24 | E-S0 | 14.8 | 13.8 | 1.1 × 0.6 | vF * in vF, eS neb | UGC 2762, MCG 7-8-19, CGCG 541-18 |
| NGC 1465 | 03 53 31.9 | +32 29 34 | S0-a | 14.6 | 13.7 | 1.7 × 0.5 | pF, pS, R, pB * nr p | UGC 2891, MCG 5-10-3, CGCG 508-4 |
| IC 256 | 02 49 40.3 | +46 57 16 | C | 17.9 | 16.9 | 0.5 × 0.3 | cF, lE, S, 1st of 3 | 5ZW 280, no. 2 of 3 comps |
| IC 257 | 02 49 45.2 | +46 58 32 | E-S0 | 13.8 | 12.6 | 1.4 × 0.8 | eF, pS, R, v diffic, 2nd of 3 | UGC 2298, MCG 8-6-11, CGCG 554-8 |
| IC 258 | 02 49 45.9 | +41 03 07 | SB0-a | 15.0 | 14.1 | 1 × 0.6 | vF, vlbM, * 9.5 f 2' | UGC 2306, CGCG 539-107, KCPG 79B |
| IC 259 | 02 49 40.8 | +41 03 20 | E-S0 | 15.3 | 14.3 | 0.7 × 0.6 | vF, double, dist 17" | CGCG 539-106, NPM1G +40.0060, KCPG 79A |
| IC 260 | 02 51 00.9 | +46 57 18 | E3 | 14.2 | 13.2 | 1 × 0.7 | eeF, pS, 2 F st nr, 3rd of 3 | UGC 2325, MCG 8-6-14, CGCG 554-11 |
| IC 262 | 02 51 43.2 | +42 49 42 | SB0 | 14.2 | 13.2 | 1.6 × 1.4 | eeF, pS, R, bet 2 st, v diffic | UGC 2335, MCG 7-6-80, CGCG 539-114 |
| IC 265 | 02 54 43.9 | +41 39 21 | E0 | 15.6 | 14.6 | 0.7 × 0.7 | eeF, eS, R | MCG 7-7-6, CGCG 540-9, CGCG 539-127, NPM1G +41.0090 |
| IC 266 | 02 55 04.7 | +42 15 50 | S | 15.6 | 14.8 | 0.7 × 0.4 | eF, eS, R | MCG 7-7-10, CGCG 539-130, CGCG 540-12 |
| IC 275 1 | 03 00 55.7 | +44 21 01 | C M | 17.3 | 16.3 | 0.3 × 0.3 | eeF, pS, R, bet 2 st | 5ZW 309 |
| IC 275 2 | 03 00 55.9 | +44 20 46 | C | 17.5 | 16.5 | 0.2 × 0.2 | eeF, pS, R, bet 2 st | 5ZW 309 |
| IC 275 3 | 03 00 58.6 | +44 21 02 | C | 16.6 | 15.6 | 0.2 × 0.2 | eeF, pS, R, bet 2 st | 5ZW 309, NPM1G +44.0059 |
| IC 278 | 03 01 30.4 | +37 45 59 | E0 | 14.2 | 13.2 | 1.1 × 1.1 | vF, * 10 p 95", F * 12" sp | UGC 2481, MCG 6-7-32, CGCG 524-44 |
| IC 284 | 03 06 09.9 | +42 22 18 | Sd | 12.5 | 11.5 | 3.8 × 1.2 | eeF, pL, lE, D * np, bet 2 st | UGC 2531, MCG 7-7-23, CGCG 540-37, IRAS 03029+4211 |
| IC 288 | 03 07 32.8 | +42 23 16 | S? | 15.1 | 14.2 | 1 × 0.3 | vF, vS, R, 2 st nf, ? S Cl | UGC 2544, MCG 7-7-27, CGCG 540-43 |
| IC 290 | 03 09 42.8 | +40 58 30 | Sb | 15.6 | 14.8 | 1.1 × 0.2 | eeF, S, R | IC 1884, UGC 2561, CGCG 540-47 |
| IC 292 | 03 10 12.9 | +40 45 57 | Sd | 14.2 | 13.5 | 1.2 × 0.7 | eF, pS, R, * s, bet 2 st | IC 1887, UGC 2567, MCG 7-7-30, CGCG 540-49, IRAS 03069+4034 |
| IC 293 | 03 10 56.1 | +41 08 16 | E-S0 | 15.3 | 14.3 | 0.6 × 0.4 | eF, S, R | IC 1888, MCG 7-7-31, CGCG 540-53, NPM1G +40.0069 |
| IC 294 | 03 11 03.1 | +40 37 18 | SB0-a | 14.8 | 13.9 | 2.1 × 1.5 | vF, pS, irr R | IC 295, IC 296, IC 1889, UGC 2574, MCG 7-7-33, CGCG 540-54 |
| IC 295 | 03 11 03.1 | +40 37 18 | SB0-a | 14.8 | 13.9 | 2.1 × 1.5 | eF, pS, R | IC 294, IC 296, IC 1889, UGC 2574, MCG 7-7-33, CGCG 540-54 |
| IC 300 | 03 14 15.8 | +42 24 54 | S0 | 16.0 | 15.0 | 0.3 × 0.3 | eF, S, R, * 9 sp, np of 2 | |
| IC 301 | 03 14 47.7 | +42 13 23 | E0 | 14.2 | 13.2 | 0.8 × 0.8 | eF, pS, R, sf of 2 | UGC 2606, MCG 7-7-36, CGCG 540-63 |
| IC 304 | 03 15 01.4 | +37 52 55 | Sb | 14.6 | 13.8 | 1.1 × 0.7 | vF, * 76" sf, np of 2 | UGC 2609, MCG 6-8-5, CGCG 525-10, IRAS 03118+3741 |
| IC 305 | 03 15 03.7 | +37 51 38 | E3 | 15.1 | 14.1 | 0.8 × 0.6 | vF, * 49" nf | MCG 6-8-6, CGCG 525-12, NPM1G +37.0120 |
| IC 308 | 03 16 15.9 | +41 10 53 | S0 | 15.4 | 14.2 | 1.2 × 1.2 | eF, pS, iR, r ? | UGC 2619 |
| IC 309 | 03 16 06.2 | +40 48 17 | S0 | 14.5 | 13.5 | 0.9 × 0.9 | eeF, pS, R, bet 2 st | MCG 7-7-43, CGCG 540-72 |
| IC 310 | 03 16 43.0 | +41 19 29 | S0 | 13.9 | 12.7 | 1.1 × 1.1 | vF, pS, R, 1259 and 1260 near | UGC 2624, MCG 7-7-45, CGCG 540-75, IRAS 03135+4108 |
| IC 311 | 03 16 46.8 | +40 00 15 | S? | 15.0 | 14.1 | 0.9 × 0.6 | eF, pS, iR, bet 2 st, vF * v close f | UGC 2625, CGCG 540-76 |
| IC 313 | 03 20 57.9 | +41 53 39 | E1 | 15.1 | 14.1 | 0.9 × 0.8 | eeF, vS, R, close D * nr s | UGC 2682, MCG 7-7-73, CGCG 540-111 |
| IC 316 1 | 03 21 19.9 | +41 55 43 | S M | 15.0 | 14.2 | 0.5 × 0.1 | eeF, pS, R | MCG 7-7-74, CGCG 540-112 |
| IC 316 2 | 03 21 19.9 | +41 55 55 | Sbc | 15.0 | 14.2 | 1.4 × 0.7 | eeF, pS, R | UGC 2688, CGCG 540-112, IRAS 03179+4145 |
| IC 320 | 03 25 59.2 | +40 47 21 | SBab | 14.5 | 13.7 | 1.2 × 1.1 | eF, pS, R, vF * close p | UGC 2732, MCG 7-8-7, CGCG 541-6 |
| IC 1874 | 03 06 21.9 | +36 00 54 | SB0-a | 14.6 | 13.7 | 1 × 0.7 | F, vS, vlbM, dif | MCG 6-7-39, CGCG 524-50, NPM1G +35.0087 |
| IC 1900 | 03 15 55.2 | +37 09 17 | S0 | 15.0 | 14.0 | 0.5 × 0.4 | F, S, pR, gbMN | MCG 6-8-7, CGCG 525-13, NPM1G +36.0098 |
| IC 1901 | 03 16 02.5 | +37 06 47 | Sa | 15.7 | 14.9 | 0.8 × 0.2 | F, vS, R, gbMN | MCG 6-8-8, CGCG 525-14, NPM1G +36.0099 |
| IC 1902 | 03 16 12.4 | +37 10 41 | S0-a | 15.5 | 14.6 | 0.4 × 0.4 | F, vS, R, sbM * 14 | CGCG 525-15, NPM1G +36.0100 |
| IC 1934 | 03 31 13.9 | +42 47 34 | S0 | 15.0 | 14.0 | 1.2 × 0.5 | eF, pS, lbM, * 12 dist 34" | UGC 2769 |
| IC 2005 | 03 57 39.5 | +36 47 15 | S | 15.6 | 14.8 | 0.4 × 0.1 | F, vS, R, stell | CGCG 526-15, "in" N 1499 |
| IC 2027 | 04 06 39.6 | +37 06 57 | E0 | 15.1 | 14.1 | 0.4 × 0.4 | F, vS, R, vlbM | UGC 2957, MCG 6-9-19 |
| PNG | RA J2000.0 | Dec J2000.0 | Main ID | PK | IRAS | Discoverer | Identities | oDiam ["] | rDiam ["] | Dist [kpc] | Rvel [km/s] | ExpVel [km/s] | C* Name | C* Mag | C* SP Type |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| PN G130.9-10.5 | 01 42 21 | +51 34 07 | NGC 650-51 | 130-10.1 | 01391+5119 | CURTIS 1918 | ARO 2, M 76, VV 6, VV'9 | 67. | 100. | 1.2 | -19.1 ± 1.2 | 38.5 (O-III), 40. (N-II) | AG82 11 | ||
| PN G133.1-08.6 | 01 58 49 | +52 53 44 | M 1- 2 | 133-08.1 | 01555+5239 | MINKOWSKI 1946 | VV 8, ARO 116, VV' 11 | 18. : | -12.1 ± 2.0 | 18.0 (O-III) | AG82 13, CSI +52-01555 0, LS V +52 1, V741 Per | B: 15.17, V: 13.44 | O + G2 Ib | ||
| PN G141.7-07.8 | 02 52 13 | +50 35 53 | A 5 | 141-07.1 | ABELL 1955 | A55 4, ARO 206, VV' 14 | 127. | 15. (N-II) | AG82 16 | U: 20.6, B: 21.4, V: 21.4 | |||||
| PN G144.3-15.5 | 02 45 26 | +42 32 36 | A 4 | 144-15.1 | 02421+4222 | ABELL 1964 | ARO 205, VV' 13 | 20. | AG82 15 | B: 19.9 | |||||
| PN G147.4-02.3 | 03 41 43 | +52 17 01 | M 1- 4 | 147-02.1 | 03379+5207 | MINKOWSKI 1946 | ARO 209, VV 11, VV' 17 | 4. | 6.0 | 2.3 : | -33.0 ± 3.9 | 13.0 (O-III) | AG82 22 | V: 16.7 | |
| PN G149.4-09.2 | 03 27 15 | +45 24 20 | HDW 3 | HARTL et al 1983 | HaWe 4 | 540. | AG82 20 | U: 16.0, B: 16.9, V: 17.0 | |||||||
| PN G149.7-03.3 | 03 49 06 | +50 00 15 | IsWe 1 | ISHIDA et al 1987 | 780. | -1.5 ± 0.5 | 5. (O-III) | U: 15.71, B: 16.45, V: 16.56 | O(C) | ||||||
| PN G151.4+00.5 | 04 13 27 | +51 51 02 | K 3-64 | KOHOUTEK 1969 | 7.5 | ||||||||||
| PN G153.7-01.4 | 04 15 55 | +48 49 41 | K 3-65 | 04122+4842 | KOHOUTEK 1969 | 2. | 5. | ||||||||
| PN G156.9-13.3 | 03 45 27 | +37 48 48 | HaWe 5 | HARTL et al 1987 | 34. | B: 17.1, V: 17.7 | |||||||||
| PN G159.0-15.1 | 03 47 33 | +35 02 49 | IC 351 | 159-15.1 | 03443+3453 | BARNARD 1891 | ARO 19, VV 12, VV' 18 | 7. | 7.0 | -9.1 ± 1.4 | 15.0 (O-III) | AG82 23 | B: 15.9, V: 15.8 | WR-Of | |
| PN G160.5-00.5 | 04 46 43 | +44 28 01 | We 1- 2 | WEINBERGER 1977 | 92. | AG82 36 | U: 20.37, B: 21.33, V: 20.87 | ||||||||
| PN G161.2-14.8 | 03 56 22 | +33 52 31 | IC 2003 | 161-14.1 | 03531+3343 | HUBBLE 1920 | ARO 76, VV 15, VV' 21 | 8.6 | 9. | -15.5 ± 2.2 | 21.5 (O-III) | AG82 25 | B: 14.7, V: 15.0 | WC 7-8, WC early, O VI | |
| PN G165.5-06.5 | 04 39 48 | +36 45 43 | K 3-67 | 04364+3639 | KOHOUTEK 1969 | 0. | 2.2 | -77.0 ± 1.4 | 20.5 (O-III), 22.5 (N-II) | AG82 34 | B: 18.5 | O(C) | |||
| PN G167.4-09.1 | 04 36 37 | +33 39 30 | K 3-66 | 04333+3333 | KOHOUTEK 1969 | 0. | 2.1 | -67.5 ± 1.7 | 16.5 (O-III), 30.5 (N-II) | AG82 32 | B: 16.26, V: 15.36 | Contin. |