Kataloge

Hercules / Milky Way Globular Clusters

«A Catalog of Parameters for Globular Clusters in the Milky Way» William E. Harris, 1996 [148]
ID Name RA Dec RSun RGC Fe/H wt EB-V VHB (m-M)V Vt MV,t U-B B-V V-R V-I spt ellip vr vLSR sigv c rc rh μV ρ0 lg(tc) lg(th)
Pal 14 AvdB 16 11 00.6 +14 57 28 76.5 71.6 -1.62 4 0.04 20.10 19.54 14.74 -4.80 72.3 ± 0.2 87.0 0.4 ± 0.1 0.80 0.82 1.22 25.25 -0.97 9.85 10.02
NGC 6205 M 13 16 41 41.24 +36 27 35.5 7.1 8.4 -1.53 13 0.02 14.90 14.33 5.78 -8.55 -0.02 0.68 0.86 F6 0.11 -244.2 ± 0.2 -228.0 7.1 ± 0.4 1.53 0.62 1.69 16.59 3.55 8.51 9.30
NGC 6229 16 46 58.79 +47 31 39.9 30.5 29.8 -1.47 2 0.01 18.03 17.45 9.39 -8.06 -0.03 0.70 1.01 F7 0.05 -154.2 ± 7.6 -138.4 1.50 0.12 0.36 16.77 3.54 8.30 9.15
NGC 6341 M 92 17 17 07.39 +43 08 09.4 8.3 9.6 -2.31 8 0.02 15.10 14.65 6.44 -8.21 0.01 0.63 0.88 F2 0.10 -120.0 ± 0.1 -103.5 6.0 ± 0.4 1.68 0.26 1.02 15.47 4.30 7.96 9.02

Legend

Key to columns [148]
ID Cluster identification number
Name Other commonly used cluster name
RA Right ascension (epoch J2000)
Dec Declination (epoch J2000)
RSun Distance from Sun (kiloparsecs)
RGC Distance from Galactic center (kpc), assuming R_0=8.0 kpc
Fe/H Metallicity [Fe/H]
wt Weight of mean metallicity; essentially the number of independent [Fe/H] measurements averaged together.
EB-V Foreground reddening
VHB V magnitude level of the horizontal branch (or RR Lyraes)
(m-M)V Apparent visual distance modulus
Vt Integrated V magnitude of the cluster
MV,t Absolute visual magnitude (cluster luminosity), M_V,t = V_t - (m-M)V
U-B Integrated color indices (uncorrected for reddening)
B-V Integrated color indices (uncorrected for reddening)
V-R Integrated color indices (uncorrected for reddening)
V-I Integrated color indices (uncorrected for reddening)
spt Spectral type of the integrated cluster light
ellip Projected ellipticity of isophotes, e = 1-(b/a)
vr Heliocentric radial velocity (km/s)
vLSR Radial velocity relative to Solar neighborhood LSR
sigv Central velocity dispersion sig_v (km/s)
c King-model central concentration, c = log(r_t/r_c); a 'c' denotes a core-collapsed cluster
rc Core radius in arcmin
rh Half-light radius in arcmin
μV Central surface brightness, V magnitudes per square arcsecond
ρ0 Central 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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