Catalogues

Serpens / Milky Way Globular Clusters

«A Catalog of Parameters for Globular Clusters in the Milky Way» William E. Harris, 1996 [148]
IDNameRADecRSunRGCFe/HwtEB-VVHB(m-M)VVtMV,tU-BB-VV-RV-IsptellipvrvLSRsigvcrcrhμVρ0lg(tc)lg(th)
Pal 515 16 05.25-00 06 41.823.218.6-1.4120.0317.5116.9211.75-5.17-58.7 ± 0.2-48.01.1 ± 0.20.52 2.292.7324.64-0.589.819.82
NGC 5904M 515 18 33.22+02 04 51.77.56.2-1.29110.0315.0714.465.65-8.810.170.720.450.95F70.1453.2 ± 0.464.35.5 ± 0.41.73 0.441.7716.093.888.289.41
NGC 653918 04 49.68-07 35 09.17.83.0-0.6351.0218.3317.629.33-8.291.011.832.23G40.0831.0 ± 1.744.41.74 0.381.7018.584.158.319.32
IC 1276Pal 718 10 44.20-07 12 27.45.43.7-0.7511.0817.7017.0110.34-6.671.031.76155.7 ± 1.3169.21.33 1.012.3821.602.788.469.03

Legend

Key to columns [148]
IDCluster identification number
NameOther commonly used cluster name
RARight ascension (epoch J2000)
DecDeclination (epoch J2000)
RSunDistance from Sun (kiloparsecs)
RGCDistance from Galactic centre (kpc), assuming R_0=8.0 kpc
Fe/HMetallicity [Fe/H]
wtWeight of mean metallicity; essentially the number of independent [Fe/H] measurements averaged together.
EB-VForeground reddening
VHBV magnitude level of the horizontal branch (or RR Lyraes)
(m-M)VApparent visual distance modulus
VtIntegrated V magnitude of the cluster
MV,tAbsolute visual magnitude (cluster luminosity), M_V,t = V_t - (m-M)V
U-BIntegrated colour indices (uncorrected for reddening)
B-VIntegrated colour indices (uncorrected for reddening)
V-RIntegrated colour indices (uncorrected for reddening)
V-IIntegrated colour indices (uncorrected for reddening)
sptSpectral type of the integrated cluster light
ellipProjected ellipticity of isophotes, e = 1-(b/a)
vrHeliocentric radial velocity (km/s)
vLSRRadial velocity relative to Solar neighborhood LSR
sigvCentral velocity dispersion sig_v (km/s)
cKing-model central concentration, c = log(r_t/r_c); a 'c' denotes a core-collapsed cluster
rcCore radius in arcmin
rhHalf-light radius in arcmin
μVCentral surface brightness, V magnitudes per square arcsecond
ρ0Central luminosity density, log_10(Solar luminosities per cubic parsec)
lg(tc)Core relaxation time t(r_c), in log_10(years)
lg(th)Median relaxation time t(r_h), in log_10(years)

References