Abell 70 with Galaxy PMN J2033-0656
History
The annular planetary nebula Abell 70 was discovered on the «Palomar Observatory Sky Survey» photo plates by George Abell in 1955. The designation in the first publication was A55 57 and in the second A66 70. [331, 332]
Physical Properties
It is a very special deep-sky object: At its northern edge it is illuminated by a spindle-shaped background galaxy. The galaxy, which is probably several million light-years away from us, appears to be about the same size in length as the relatively close PN, which happens to be in the line of sight between us and the distant galaxy. Distance estimates from Abell 70 range from 2.4 to 3.5 kiloparsecs. The PN is moving towards us at a radial speed of around 79 km/s. Measurements of the expansion speed based on the OIII lines showed that the nebula expands at 38 km/s. [141]
| Designations | PN G038.1-25.4: A 70, PK 38-25.1, A55 57, ARO 351, VV' 536 |
| Right Ascension (J2000.0) | 20h 31m 33s |
| Declination (J2000.0) | -07° 05' 21" |
| Dimensions | 42." (optical) |
| Radial Velocity | -79.0 km/s ± 18.0 km/s |
| Expansion Velocity | 37.8 km/s (O-III) |
| C-Star Designations | AG82 410 |
| C-Star Magnitude | 19.1 mag (B filter) |
| Discoverer | ABELL 1955 |
Galaxie PMN J2033-0656
The galaxy behind the northern edge of the PN is apparently a radio galaxy with the designation PMN J2033-0656 from the Parkes-MIT-NRAO Survey - this according to the information from the NASA Extragalactic Database (NED), which refers to an article in APJS (1995, 97, p.347, Griffith). Other names are 2MASX J20313312-0705014 or WISEA J203133.10-070501.5. The redshift z is 0.019423, which corresponds to a speed of 5823 km/s.
Further infos at CDS: 2MASX J20313312-0705014
Finder Chart
The unequal pair lies between the constellations Aquila (Eagle) and Aquarius (Water Bearer). A good starting point is the 3.8 mag bright star Albali (ε Aquarii). About 4.5 degrees northwest of it in the direction of θ Aquilae you will experience an unusual encounter. A large telescope aperture and a dark sky are essential for the visual observation of this fine pair of objects. This object is best observed in the months of August to October.
Visual Observation
Pending ...