scholarly journals Globular cluster systems in low-luminosity early-type galaxies near the Fornax cluster centre

2006 ◽  
Vol 367 (1) ◽  
pp. 156-168 ◽  
Author(s):  
Lilia P. Bassino ◽  
Tom Richtler ◽  
Boris Dirsch
2011 ◽  
Vol 728 (2) ◽  
pp. 116 ◽  
Author(s):  
Chengze Liu ◽  
Eric W. Peng ◽  
Andrés Jordán ◽  
Laura Ferrarese ◽  
John P. Blakeslee ◽  
...  

2012 ◽  
Vol 429 (2) ◽  
pp. 1066-1079 ◽  
Author(s):  
R. Smith ◽  
R. Sánchez-Janssen ◽  
M. Fellhauer ◽  
T. H. Puzia ◽  
J. A. L. Aguerri ◽  
...  

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.


2013 ◽  
Vol 769 (2) ◽  
pp. 145 ◽  
Author(s):  
Qiushi Wang ◽  
Eric W. Peng ◽  
John P. Blakeslee ◽  
Patrick Côté ◽  
Laura Ferrarese ◽  
...  

2010 ◽  
Vol 710 (2) ◽  
pp. 1672-1682 ◽  
Author(s):  
Steffen Mieske ◽  
Andrés Jordán ◽  
Patrick Côté ◽  
Eric W. Peng ◽  
Laura Ferrarese ◽  
...  

1996 ◽  
Vol 171 ◽  
pp. 438-438
Author(s):  
M. Kissler-Patig ◽  
S. Kohle ◽  
M. Hilker ◽  
T. Richtler ◽  
L. Infante ◽  
...  

We present V and I photometry of the globular cluster systems of the early-type galaxies NGC 1374, NGC 1379, NGC 1387, NGC 1427, and NGC 1399, obtained with the 100 inch telescope of Las Campanas Observatory.


2002 ◽  
Vol 207 ◽  
pp. 281-286
Author(s):  
Michael Hilker

In this contribution, first results of deep VLT (V,I) photometry in the central region of the Hydra I galaxy cluster are presented. Many star clusters have been identified not only around several early-type galaxies, but also in the intra-cluster field, as far as 250 kpc from the cluster center. Outside the bulges of the central galaxies NGC 3311 and NGC 3309, the intra-cluster globular cluster system is dominated by blue clusters whose spatial distribution is similar to that of the (newly discovered) dwarf galaxies in Hydra I. The color distributions of globular clusters around NGC 3311 and NGC 3309 are multimodal, with a sharp blue peak and a slightly broader distribution of the red cluster population.


2006 ◽  
Vol 463 (2) ◽  
pp. 493-502 ◽  
Author(s):  
M. Hempel ◽  
M. Kissler-Patig ◽  
T. H. Puzia ◽  
M. Hilker

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