{ "id": "1601.05054", "version": "v1", "published": "2016-01-19T19:58:26.000Z", "updated": "2016-01-19T19:58:26.000Z", "title": "Correlation between lithium abundances and ages of solar twin stars", "authors": [ "Marilia Carlos", "Poul E. Nissen", "Jorge Melendez" ], "comment": "6 pages and 6 figures. Submitted to Astronomy & Astrophysics", "categories": [ "astro-ph.SR" ], "abstract": "We want to determine the lithium abundances of solar twin stars as a function of stellar age to provide constraints for stellar evolutions models and to investigate whether there is a connection between low Li abundance and the occurrence of planets. For a sample of 21 solar twins observed with the HARPS spectrograph at high spectral resolution (R~115.000) and very high signal-to-noise ratio (600 < S/N < 2400), precise lithium abundances were obtained by spectral synthesis of the LiI 6707.8 A line and compared to stellar ages, masses, and metallicities determined from a spectroscopic analysis of the same set of HARPS spectra. We show that for the large majority of the solar twins there is a strong correlation between lithium abundance and stellar age. As the age increases from 1 to 9 Gyr, the Li abundance decreases by a factor of ~ 50. The relation agrees fairly well with predictions from non-standard stellar evolution models of Li destruction at the bottom of the upper convection zone. Two stars deviate from the relation by having Li abundances enhanced by a factor of ~ 10, which may be due to planet engulfment. On the other hand, we find no indication of a link between planet hosting stars and enhanced lithium depletion.", "revisions": [ { "version": "v1", "updated": "2016-01-19T19:58:26.000Z" } ], "analyses": { "keywords": [ "solar twin stars", "stellar age", "correlation", "non-standard stellar evolution models", "upper convection zone" ], "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable" } } }