YNAO OpenIR  > 大样本恒星演化研究组
The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia
Meng XC(孟祥存)1,2; Han ZW(韩占文)1,2; Meng, XC
发表期刊ASTRONOMY & ASTROPHYSICS
2016-04-01
卷号588
DOI10.1051/0004-6361/201526077
产权排序第1完成单位
收录类别SCI ; EI
关键词Binaries: Symbiotic Stars: Evolution Supernovae: General White Dwarfs
摘要Context. Symbiotic systems (i.e. a white dwarf + red giant star, WD + RG), which experience mass loss and form circumstellar material (CSM), have been suggested as being a possible progenitor system of type Ia supernovae (SNe Ia). After a supernova explosion, the supernova ejecta may interact with the CSM or the RG secondary. X-ray/radio emission (excess UV photons) is expected from the interaction between supernova ejecta and the CSM (RG secondary). However, no X-ray or radio emission that has originated from this type of system has been observationally detected, and only four SNe Ia have shown any possible signal of excess UV emission. These observational discrepancies need to be interpreted.
项目资助者NSFC(11473063, 11522327, 11390374, 11521303) ; CAS "Light of West China" Program ; CAS(KJZD-EW-M06-01) ; Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09010202) ; Science and Technology Innovation Talent Programme of the Yunnan Province(2013HA005)
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-6361
URL查看原文
归档日期2016-12-30
WOS记录号WOS:000373207800100
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SINGLE-DEGENERATE CHANNEL ; KEPLERS SUPERNOVA REMNANT ; CHANDRASEKHAR MASS MODELS ; ASYMPTOTIC-GIANT-BRANCH ; LONG DELAY TIMES ; RAY-EMISSION ; STELLAR EVOLUTION ; WHITE-DWARFS ; CIRCUMSTELLAR MATERIAL ; RADIO-EMISSION
引用统计
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9585
专题大样本恒星演化研究组
中国科学院天体结构与演化重点实验室
通讯作者Meng, XC
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, PR China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650216 Kunming, PR China
推荐引用方式
GB/T 7714
Meng XC,Han ZW,Meng, XC. The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia[J]. ASTRONOMY & ASTROPHYSICS,2016,588.
APA Meng XC,Han ZW,&Meng, XC.(2016).The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia.ASTRONOMY & ASTROPHYSICS,588.
MLA Meng XC,et al."The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia".ASTRONOMY & ASTROPHYSICS 588(2016).
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
The X-ray_radio and (486KB)期刊论文作者接受稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Meng XC(孟祥存)]的文章
[Han ZW(韩占文)]的文章
[Meng, XC]的文章
百度学术
百度学术中相似的文章
[Meng XC(孟祥存)]的文章
[Han ZW(韩占文)]的文章
[Meng, XC]的文章
必应学术
必应学术中相似的文章
[Meng XC(孟祥存)]的文章
[Han ZW(韩占文)]的文章
[Meng, XC]的文章
相关权益政策
暂无数据
收藏/分享
文件名: The X-ray_radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。