RCW 120中尘埃的数值模型
星系天体物理
2019-11-20 v1
摘要
在一颗O型速逃星周围观测到的星际气泡RCW 120,由该星发出的星风和电离辐射驱动。星风与星际介质(ISM)之间的边界,与HII区内该星周围弧形的中红外尘埃发射相关。
引用
@article{arxiv.1909.07150,
title = {Numerical models for the dust in RCW 120},
author = {A. Rodríguez-González and Z. Meliani and M. Sánchez-Cruces and P. R. Rivera-Ortiz and A. Castellanos-Ramírez},
journal= {arXiv preprint arXiv:1909.07150},
year = {2019}
}
备注
6 pages, 5 figures, 1 table, accepted for publication in A&A