Circumstellar interaction in Type IIn supernovae

被引：0
作者：
Chandra, Poonam [1 ]
Chevalier, Roger A. [2 ]
Chugai, Nikolai [3 ]
Soderberg, Alicia M. [4 ]
Fransson, Claes [5 ]
机构：
[1] Pune Univ Campus, Nat Ctr Radio Astrophys, Pune 411007, Maharashtra, India
[2] Univ Virginia, Dept Astron, Charlottesville, VA 22904 USA
[3] Russian Acad Sci, Inst Astron, Moscow 109017, Russia
[4] Smithsonian Astrophys Observ, Cambridge, MA 02138 USA
[5] Stockholm Univ, Dept Astron, SE-10691 Stockholm, Sweden
来源：
SUPERNOVA ENVIRONMENTAL IMPACTS | 2014年 / 9卷 / S296期
关键词：
dense matter; radiation mechanisms: general; circumstellar matter; stars: mass loss; supernovae:; individual; (2006jd; 2010jl); X-RAY; RADIO-EMISSION; SN-1988Z;
D O I：
10.1017/S1743921313009368
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Type IIn supernovae have bright optical emission and high bolometric luminosities. Due to their high mass loss, their are expected to have dense circumstellar interaction, thus produce bright radio and X-ray emission. We aim to carry out systematic study to understand their circumstellar interaction, mass loss properties. Here, I provide specific examples of two Type IIn supernovae, 2006jd and 2010jl.
引用
收藏
页码：135 / 143
页数：9
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