期刊
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
卷 121, 期 881, 页码 689-698出版社
UNIV CHICAGO PRESS
DOI: 10.1086/603653
关键词
-
资金
- National Science Foundation [AST-0607485]
- FONDAP [15010003]
- [68.D-0571(A)]
- [69.D-0438(A)]
- [170.A-0519(A)]
- [68.A-0443]
- [P06-045-F]
- [PFB 06/09]
Here we present previously unpublished optical spectra of supernova (SN) 2001ig, a Type IIb SN, from about a week after explosion until nearly one year later. The earliest spectrum consists of only a few broad absorption features, but soon more common Type II SN features including hydrogen P Cygni profiles and helium absorption become apparent. At later times, as the H features fade and the He I absorption becomes more prominent, we observe the SN to transition from a Type II to a Type Ib. Finally, observations after 250 days past explosion show a nebular-phase SN spectrum with one of the largest magnesium to oxygen intensity ratios ever seen. Additionally, we present models of the late-time spectra which indicate that the inner ejecta consist of similar to 1.15 M(circle dot) of material, most of which (by mass) is in the form of oxygen, with similar to 0.13 M(circle dot) of (56)Ni and essentially no hydrogen.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据