红巨星三维大气模型
太阳与恒星天体物理
2015-05-30 v1
摘要
我们利用三维辐射流体力学代码 CO5BOLD，简要概述了红巨星大气层的建模工作。我们强调了三维建模在标准静力学一维模型之外所提供的额外见解，并对当前的建模挑战进行了评论。
引用
@article{arxiv.1108.4554,
title = {3D Model Atmospheres of Red Giant Stars},
author = {Hans-Gunter Ludwig and Matthias Steffen},
journal= {arXiv preprint arXiv:1108.4554},
year = {2015}
}
备注
Proc. of the workshop "Red Giants as Probes of the Structure and Evolution of the Milky Way" (Roma, 15-17 Nov 2010), Astrophysics and Space Science Proceedings, ISBN 978-3-642-18417-8 (eds. A. Miglio, J. Montalban, A. Noels). Part of RedGiantsMilkyWay/2011/ proceedings available at http://arxiv.org/html/1108.4406v1