{ "id": "1501.00874", "version": "v1", "published": "2015-01-05T14:15:33.000Z", "updated": "2015-01-05T14:15:33.000Z", "title": "Mass loss on the red giant branch: the value and metallicity dependence of Reimers' η in globular clusters", "authors": [ "Iain McDonald", "Albert Zijlstra" ], "comment": "Accepted MNRAS", "categories": [ "astro-ph.SR" ], "abstract": "The impact of metallicity on the mass-loss rate from red giant branch (RGB) stars is studied through its effect on the parameters of horizontal branch (HB) stars. The scaling factors from Reimers (1975) and Schroder & Cuntz (2005) are determined for 56 well-studied Galactic globular clusters (GCs). The median values among clusters are, respectively, {\\eta}_R = 0.477 +/- 0.070 (+0.050/-0.062) and {\\eta}_SC = 0.172 +/- 0.024 (+0.018/-0.023) (standard deviation and systematic uncertainties, respectively). Mass-loss mechanisms on the RGB have very little metallicity dependence: over a factor of 200 in iron abundance, {\\eta} varies by <~30 per cent, within the current systematic uncertainties on cluster ages and evolution models. Since {\\eta} incorporates cluster age, the low standard deviation of {\\eta} among clusters (~14 per cent) suggests that age can almost entirely account for the \"second parameter problem\". The remaining spread in {\\eta} correlates with cluster mass and density, suggesting helium enrichment provides the third parameter explaining HB morphology of GCs. The metallicity variation is reduced further if globular clusters are more co-eval than generally thought. This would also better reproduce the observed AGB tip luminosities, which are not well modelled by extrapolating the RGB {\\eta} to later evolutionary epochs.", "revisions": [ { "version": "v1", "updated": "2015-01-05T14:15:33.000Z" } ], "analyses": { "keywords": [ "red giant branch", "globular clusters", "metallicity dependence", "mass loss", "third parameter explaining hb morphology" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }