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

页码：135 / 143

页数：9

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