Indication of the High Mass-Transfer Ratio in S-type Symbiotic Binaries
Solar and Stellar Astrophysics
2017-03-20 v1
Abstract
By modelling H column densities in eclipsing S-type symbiotic stars EG And and SY Mus, we derived the wind velocity profile and the corresponding mass-loss rate from their giants. Our analysis revealed a strong enhancement of the wind at the orbital plane.
Keywords
Cite
@article{arxiv.1602.01668,
title = {Indication of the High Mass-Transfer Ratio in S-type Symbiotic Binaries},
author = {Natalia Shagatova and Augustin Skopal},
journal= {arXiv preprint arXiv:1602.01668},
year = {2017}
}
Comments
proceedings of the conference "The Physics of Evolved Stars: a Conference Dedicated to the Memory of Olivier Chesneau", 2 pages, 2 figures