Catalogues

Hercules / 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 14AvdB16 11 00.6+14 57 2876.571.6-1.6240.0420.1019.5414.74-4.8072.3 ± 0.287.00.4 ± 0.10.80 0.821.2225.25-0.979.8510.02
NGC 6205M 1316 41 41.24+36 27 35.57.18.4-1.53130.0214.9014.335.78-8.55-0.020.680.86F60.11-244.2 ± 0.2-228.07.1 ± 0.41.53 0.621.6916.593.558.519.30
NGC 622916 46 58.79+47 31 39.930.529.8-1.4720.0118.0317.459.39-8.06-0.030.701.01F70.05-154.2 ± 7.6-138.41.50 0.120.3616.773.548.309.15
NGC 6341M 9217 17 07.39+43 08 09.48.39.6-2.3180.0215.1014.656.44-8.210.010.630.88F20.10-120.0 ± 0.1-103.56.0 ± 0.41.68 0.261.0215.474.307.969.02

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