Further progress on solar age calibration
Astrophysics
2015-05-13 v1
Abstract
We recalibrate a standard solar model seismologically to estimate the main-sequence age of the Sun. Our procedure differs from what we have done in the past by removing from the observed frequencies the effect of hydrogen ionization and the superadiabatic convective boundary layer. Our preliminary result is Gy.
Keywords
Cite
@article{arxiv.0812.5044,
title = {Further progress on solar age calibration},
author = {Günter Houdek and Douglas Gough},
journal= {arXiv preprint arXiv:0812.5044},
year = {2015}
}
Comments
Accepted for publication in Comm. Asteroseis., 2 pages, 1 figure