|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
S98 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
Plots (from earlier versions of the table):
Globular cluster colours vs galaxy velocity dispersion (full sample). Figure 1
Globular cluster colours vs galaxy velocity dispersion (error = +/- 0.03 sample). Figure 2
Globular cluster colours vs galaxy absolute magnitude (full sample). Figure 3
An electronic version of the table can be obtained by emailing dforbes@swin.edu.au
Notes:
Galaxy name; Distance modulus
from PS96,
includes Virgocentric infall correction and Ho = 75 km/s/Mpc; M_V
is total V band absolute magnitude from PS96
after Galactic extinction correction of S98;
Galaxy central velocity dispersion from PS96
(Milky Way velocity dispersion comes from K92
); Mean S98
extinction-corrected V-I colour for the blue globular clusters
and estimated error; Mean S98
extinction-corrected V-I colour for the red globular clusters and estimated
error; Reference for the globular cluster data; Bimodal
colour distribution (Y=Yes or L=Likely); Original colour system (transformed to V-I
using FF00 or
BH00 for
[Fe/H]); Observations (H=HST or G=Ground).
References:
L01
: Larsen
et al. , 2001, AJ, 121, 2974.
K99
: Kundu, 1999, PhD Thesis
F01
: Forbes, Georgakakis, Brodie,
2001, MNRAS, 325, 1431.
K97
: Kissler-Patig et al. , 1997, A&A, 327, 503
F98
: Forbes et al. , 1998, MNRAS, 293, 325
F01
: Forte et al., 2001, AJ, 121, 1992
BF00
: Brown, Forbes, et al. , 2000, MNRAS, 317, 406
B00
: Brodie et al. , 2000, ApJ, 543, L19
Z95
: Zepf et al. , 1995, ApJ ,443, 570
GK99
: Gebhardt , Kissler-Patig, 1999, AJ, 118, 1526
F97
: Forbes et al. , 1997, AJ ,113, 1652
GF00
: Georgakakis, Forbes, Brodie,
2000, MNRAS, 324, 785.
L00
: Larson, 2000, private comm.
F96
: Forbes et al. , 1996, ApJ, 467, 126
BH00
: Barmby et al. , 2000, AJ, 119, 727
K92
: Kent , 1992, ApJ 387, 181
S98
: Schlegel et al. , 1998, ApJ, 500, 525
PS96
: Prugniel, Simien, 1996, A&A, 309, 749
FF00
: Forbes, Forte, 2000, MNRAS,
322, 257.
R01
: Rejkuba 2001, A&A, 369, 812.
D01
: Da Rocha etal., 2002, AJ, 123, 690.
G03
: Gomez, Richtler 2003, A&A, 415, 499.
D03
: Dirsch etal 2003, A&A, 408, 929.
D05
: Dirsch etal 2005, A&A, 433, 43
F06
: Forbes etal 2006, MNRAS, 366, 1230.
B06
: Bassino etal 2006, MNRAS in press.
W02
: Whitmore etal 2002, AJ, 124, 147.
G04
: Goudfrooij etal 2004, ApJ, 613, 121.
H06
: Harris etal 2006, ApJ, 636, 90.