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

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

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hia....13..202k&link_type=abstract

Highlights of Astronomy, Vol. 13, as presented at the XXVth General Assembly of the IAU - 2003 [Sydney, Australia, 13 - 26 July

Astronomy and Astrophysics

Astronomy

Scientific paper

Formation of metal-rich globular cluster populations (MRGCPs) in the bulges of spirals and ellipticals is addressed. I summarize basic results which can be indirect evidence that the formation of these populations is preferably related to certain stage of the host galaxies' (chemical?) evolution. Attention is paid to massive star cluster populations (MSCPs) in nearby (dwarf) irregulars. Mean metallicities of MSCPs preferably fall between 0.004

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