A photometric study of the X-ray globular cluster NGC 1851

1981 ◽  
Vol 86 ◽  
pp. 687 ◽  
Author(s):  
P. B. Stetson
1978 ◽  
Vol 224 ◽  
pp. 383 ◽  
Author(s):  
M. H. Liller ◽  
B. W. Carney

2018 ◽  
Vol 479 (2) ◽  
pp. 2834-2852 ◽  
Author(s):  
Simon Henleywillis ◽  
Adrienne M Cool ◽  
Daryl Haggard ◽  
Craig Heinke ◽  
Paul Callanan ◽  
...  
Keyword(s):  

2011 ◽  
Vol 732 (1) ◽  
pp. 46 ◽  
Author(s):  
W. S. Stacey ◽  
C. O. Heinke ◽  
R. F. Elsner ◽  
P. D. Edmonds ◽  
M. C. Weisskopf ◽  
...  

1997 ◽  
Vol 490 (2) ◽  
pp. L161-L164 ◽  
Author(s):  
E. V. Gotthelf ◽  
S. R. Kulkarni
Keyword(s):  

2014 ◽  
Vol 441 (1) ◽  
pp. 757-768 ◽  
Author(s):  
L. M. Forestell ◽  
C. O. Heinke ◽  
H. N. Cohn ◽  
P. M. Lugger ◽  
G. R. Sivakoff ◽  
...  

Author(s):  
A. Jordán ◽  
G.R. Sivakoff ◽  
C.L. Sarazin ◽  
J.P. Blakeslee ◽  
E.L. Blanton ◽  
...  

Author(s):  
Michel Aurière ◽  
Claude Chevalier ◽  
Sergio Ilovaisky ◽  
Lydie Koch-Miramond ◽  
Jean-Pierre Cordoni
Keyword(s):  

2002 ◽  
Vol 207 ◽  
pp. 229-237
Author(s):  
Arunav Kundu ◽  
Brad Whitmore

We present the results of our detailed WFPC2-based photometric study of the globular cluster systems (GCS) of over 60 elliptical and SO galaxies. Approximately 50% of the GCSs of ellipticals, and at least 15–20% of S0s reveal bimodality in the color distribution. We trace the variation in GCS properties with Hubble type and discuss the implications on the various models of galaxy (and cluster system) formation. We also provide evidence that the globular cluster luminosity function is an excellent distance indicator with an accuracy comparable to the surface brightness fluctuation method.


2009 ◽  
Vol 692 (1) ◽  
pp. 584-593 ◽  
Author(s):  
Craig O. Heinke ◽  
Haldan N. Cohn ◽  
Phyllis M. Lugger
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document