经典新星与再发新星的爆发
太阳与恒星天体物理
2015-05-14 v3
摘要
在这篇综述中，我介绍了我们目前对经典新星与再发新星系统的认知状况。选取了两个特定天体（V1974 Cyg 和 RS Oph）来说明可能与其爆发相关的各种现象。强调了新星研究的更广泛重要性，并总结了一些最紧迫的未解问题。
引用
@article{arxiv.0911.5254,
title = {The Outbursts of Classical and Recurrent Novae},
author = {M. F. Bode},
journal= {arXiv preprint arXiv:0911.5254},
year = {2015}
}
备注
8 pages, 4 figures. Review paper presented at the May 2009 XMM-Newton Workshop on Super-Soft X-ray Sources. Published in Astronomische Nachrichten, Vol 331, p160 (2010). Revised version: Corrected minor typographical errors to P_orb vs P_rot on p2 and estimated Galactic nova rate on p3