关于银河旋臂l-V特征的自洽恒星与气体动力学模型解释
天体物理学
2007-05-23 v1
摘要
提出一种新方案，解释了银河系中心数千光秒范围内气体的l-V分布中占主导地位的特征，基于无对称性且高分辨率的3维N体和SPH模拟。
引用
@article{arxiv.astro-ph/9711005,
title = {Interpreting the main HI and CO l-V features in the Galactic bar from self-consistent stellar and gas dynamical models},
author = {R. Fux},
journal= {arXiv preprint arXiv:astro-ph/9711005},
year = {2007}
}
备注
2 pages, LaTeX, 1 figure. To appear in Proc. IAU Symp. 184, "The Central Regions of the Galaxy and Galaxies", ed. Y. Sofue. Part of Fux 1997, PhD thesis, Geneva Observatory. Also available at http://obswww.unige.ch/Preprints/cgi-bin/Preprintshtml.cgi?#DYNAMIC