Kataloge

Norma / 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)
NGC 594615 35 28.52-50 39 34.810.65.8-1.2940.5417.4016.799.61-7.180.451.290.771.58F7/80.16128.4 ± 1.8128.94.0 ± 2.92.50 c0.080.8917.194.686.908.91
BH 17615 39 07.45-50 03 09.818.912.90.0010.5418.8618.0614.00-4.060.85 0.900.9023.360.979.148.79
Lynga 7BH18416 11 03.65-55 19 04.08.04.3-0.6730.7317.4316.7810.18-6.608.0 ± 5.08.00.95 0.901.208.83

Legende

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)

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