SN 2011ht: A weak explosion in a massive extended envelope

被引:10
作者
Chugai, N. N. [1 ]
机构
[1] Russian Acad Sci, Inst Astron, Ul Pyatnitskaya 48, Moscow 119017, Russia
来源
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2016年 / 42卷 / 02期
关键词
supernovae; nucleosynthesis; SUPERNOVA; EVOLUTION; EMISSION; 1994W;
D O I
10.1134/S106377371602002X
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The possibility of explaining the light curve and the low expansion velocity of SN 2011ht, which belongs to a group of three objects showing signatures of both type IIn and type IIP supernovae, is explored. The radiated energy and expansion velocity of the ejecta of SN 2011ht are shown to be consistent with a low-energy supernova explosion (a parts per thousand 6 x 10(49) erg) and a parts per thousand currency sign2 ejecta expanding within a circumstellar envelope of radius similar to 2 x 10(14) cm and mass 6-8 An observational test for this scenario is proposed.
引用
收藏
页码:82 / 89
页数:8
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