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

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

2001-06-13

arxiv.org/abs/astro-ph/0106227v1

Astronomy and Astrophysics

Astrophysics

2 pages, no figures, uses IAU207_pasp.sty. To be published in the Proceedings of the IAU Symposium 207, "Extragalactic Star Cl

Scientific paper

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 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.

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