Self-Induced Formaton of Metal-Rich Globulars in Bulges?
Astrophysics
2007-05-23 v1
Abstract
Taken together, key latest observations assume that (i) old metal-rich globular cluster populations (MRGCPs) in bulges were able to form due to essentially increased, self(internally)-induced star formation rate (SFR) in the hosts, while galaxy merging played an additional role; (ii) massive star cluster populations (MSCPs) in irregulars may be young, less prominent counterparts of the old MRGCPs in spheroids.
Cite
@article{arxiv.astro-ph/0309531,
title = {Self-Induced Formaton of Metal-Rich Globulars in Bulges?},
author = {Valery V. Kravtsov},
journal= {arXiv preprint arXiv:astro-ph/0309531},
year = {2007}
}
Comments
1 page, no figures, poster presenrted at JD06, IUA General Assembly, Sydney, July 17, 2003, to appear in Highlights of Astronomy