中文

II型超新星的光谱建模

天体物理学 2008-11-26 v1

摘要

我们利用对SN IIP 2005cs的模型,展示了详细的光谱分析可用于确定红化程度和元素丰度。

关键词

引用

@article{arxiv.astro-ph/0611545,
  title  = {Spectral Modeling of Type II Supernovae},
  author = {E. Baron},
  journal= {arXiv preprint arXiv:astro-ph/0611545},
  year   = {2008}
}

备注

8 pages, 7 figures. To appear in The Multicoloured Landscape of Compact Objects and their Explosive Progenitors: Theory vs Observations, eds, L. Burderi et al. (New York: AIP)