Solar System chemical abundances corrected for systematics
Solar and Stellar Astrophysics
2015-06-19 v1
Abstract
The relative chemical abundances between CI meteorites and the solar photosphere exhibit a significant trend with condensation temperature. A trend with condensation temperature is also seen when the solar photospheric abundances are compared to those of nearby solar twins. We use both these trends to determine the alteration of the elemental abundances of the meteorties and the photosphere by fractionation and calculate a new set of primordial Solar System abundances.
Cite
@article{arxiv.1406.0480,
title = {Solar System chemical abundances corrected for systematics},
author = {Guillermo Gonzalez},
journal= {arXiv preprint arXiv:1406.0480},
year = {2015}
}
Comments
5 pages; letter; accepted for publication in MNRAS