Early spectra of supernovae

被引:0
|
作者
Baron, E [1 ]
Nugent, PE [1 ]
Branch, D [1 ]
Hauschildt, PH [1 ]
机构
[1] Univ Oklahoma, Dept Phys & Astron, Norman, OK 73019 USA
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We briefly describe the current version of the PHOENIX code. We then present some results on the modeling of Type II supernovae and show that fits to observations can be obtained, when account is taken for spherically symmetric, line-blanketed, expanding atmospheres. We describe the SEAM method of obtaining distances to supernovae and briefly discuss its future prospects.
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页码:351 / 357
页数:7
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