Mass Loss on the Red Giant Branch and the Second-Parameter Phenomenon

Details Mass Loss on the Red Giant Branch and the Second-Parameter Phenomenon Mass Loss on the Red Giant Branch and the Second-Parameter Phenomenon

1999-09-21

arxiv.org/abs/astro-ph/9909345v1

Astronomy and Astrophysics

Astrophysics

6 pages, 3 figures. To appear in "The Galactic Halo: from Globular Clusters to Field Stars"

Scientific paper

The "second-parameter effect" is characterized by the existence of globular clusters (GCs) with similar metallicity [Fe/H] (the "first parameter") but different horizontal-branch (HB) morphologies. One of the primary second-parameter candidates is cluster age. In the present paper, we address the following issue: "Are the age differences between second-parameter GCs, as derived from their main-sequence turnoff properties, consistent with their relative HB types?" In order to provide an answer to this question, several analytical formulae for the mass loss rate on the red giant branch are analyzed and employed. The case of M5 vs. Palomar 4/Eridanus is specifically discussed. Our results show that, irrespective of the mass loss formula employed, the relative turnoff ages of GCs are insufficient to explain the second-parameter phenomenon, unless GCs are younger than 10 Gyr.

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