Catalogues

Tucana / 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 10447 Tuc00 24 05.67-72 04 52.64.57.4-0.72100.0414.0613.373.95-9.420.370.880.531.14G40.09-18.0 ± 0.1-26.711.0 ± 0.32.07 0.363.1714.384.887.849.55
NGC 36201 03 14.26-70 50 55.68.69.4-1.2650.0515.4414.836.40-8.430.160.770.491.01F90.01223.5 ± 0.5214.06.4 ± 0.31.76 c:0.180.8214.804.747.768.93

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