Self-Induced Formaton of Metal-Rich Globulars in Bulges?

Details Self-Induced Formaton of Metal-Rich Globulars in Bulges? Self-Induced Formaton of Metal-Rich Globulars in Bulges?

2003-09-19

arxiv.org/abs/astro-ph/0309531v1

Astronomy and Astrophysics

Astrophysics

1 page, no figures, poster presenrted at JD06, IUA General Assembly, Sydney, July 17, 2003, to appear in Highlights of Astrono

Scientific paper

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.

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