{ "id": "1004.2709", "version": "v1", "published": "2010-04-15T20:05:23.000Z", "updated": "2010-04-15T20:05:23.000Z", "title": "A Bound on the Light Emitted During the TP-AGB Phase", "authors": [ "Jonathan C. Bird", "Marc H. Pinsonneault" ], "comment": "Submitted to the Astrophysical Journal. 25 pages, 2 figures.", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "The integrated luminosity of the TP-AGB phase is a major uncertainty in stellar population synthesis models. We use the white dwarf initial final mass relation and stellar interiors models to demonstrate that a significant fraction of the core mass growth for intermediate (1.5 < Msun < 6) mass stars takes place during the TP-AGB phase. We find evidence that the peak fractional core mass contribution for TP-AGB stars is ~20% and occurs for stars between 2 Msun and 3.5 Msun. Using a simple fuel consumption argument we couple this core mass increase to a lower limit on the TP-AGB phase energy output. Roughly half of the energy released in models of TP-AGB stars can be directly accounted for by this core growth; while the remainder is predominantly the stellar yield of He. A robust measurement of the emitted light in this phase will therefore set strong constraints on helium enrichment from TP-AGB stars, and we estimate the yields predicted by current models as a function of initial mass. Implications for stellar population studies and prospects for improvements are discussed.", "revisions": [ { "version": "v1", "updated": "2010-04-15T20:05:23.000Z" } ], "analyses": { "keywords": [ "tp-agb stars", "peak fractional core mass contribution", "white dwarf initial final mass", "dwarf initial final mass relation" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/733/2/81", "journal": "The Astrophysical Journal", "year": 2011, "month": "Jun", "volume": 733, "number": 2, "pages": 81 }, "note": { "typesetting": "TeX", "pages": 25, "language": "en", "license": "arXiv", "status": "editable", "inspire": 852228, "adsabs": "2011ApJ...733...81B" } } }