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Second-parameter Globular Clusters in the Milky Way and in M33 as Tracers of Mass Loss from M31 in the Early Epoch?

Published online by Cambridge University Press:  03 August 2017

Valery V. Kravtsov
Valery V. Kravtsov*
Affiliation:
Sternberg Astron. Ins., 13, University Ave., Moscow 119899, Russia

Abstract

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I suggest that the bulk of the “young”, second-parameter globular clusters (SPGCs) observed in the outer halo of our Galaxy and recently found in the other massive spiral of the Local Group (LG), M33, may have originated due to mass outflow from M31 and subsequent accretion of gas on the Galaxy and M33 in the early epoch.

Type
Part 1. The Star Clusters of Local Group Galaxies
Information
Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 163 - 164
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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