Destruction of 3He in Low Mass Stars and Implications for Chemical Evolution
Abstract
Recent observations of 3He/H in different environments tend to prove that 3He is not produced in low mass stars, contrary to the standard predictions of stellar evolution theory. We show how a simple consistent mechanism, namely rotation-induced mixing, can lead to the destruction of 3He in low mass stars and simultaneously account for the low 12C/13C ratios and low lithium abundances observed in giant stars of different populations. This process should both naturally account for the recent measurements of 3He/H in galactic HII regions and allow for high values of 3He observed in some planetary nebulae.
Cite
@article{arxiv.astro-ph/9512147,
title = {Destruction of 3He in Low Mass Stars and Implications for Chemical Evolution},
author = {C. Charbonnel},
journal= {arXiv preprint arXiv:astro-ph/9512147},
year = {2007}
}
Comments
Proceedings of the meeting "From Stars to Galaxies" Crete, 9-13 oct.1995, C.Leitherer, U.Fritze-von Alvensleben, L.Hucra eds, PASP in press, 5 pages, uuencoded, compressed Postscript file including all figures