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

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dc.creatorKravtsov, Valery V.
dc.date2003-09-19
dc.date.accessioned2026-07-07T02:09:41Z
dc.date.available2026-07-07T02:09:41Z
dc.descriptionTaken 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.
dc.description1 page, no figures, poster presenrted at JD06, IUA General Assembly, Sydney, July 17, 2003, to appear in Highlights of Astronomy
dc.identifierhttps://arxiv.org/abs/astro-ph/0309531
dc.identifierhttp://arxiv.org/abs/astro-ph/0309531
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6522
dc.subjectAstrophysics
dc.titleSelf-Induced Formaton of Metal-Rich Globulars in Bulges?
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