The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia
文献类型:期刊论文
作者 | Meng XC(孟祥存)1,2![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2016-04-01 |
卷号 | 588 |
关键词 | binaries: symbiotic stars: evolution supernovae: general white dwarfs |
ISSN号 | 1432-0746 |
产权排序 | 第一完成单位 |
通讯作者 | Meng, XC |
英文摘要 | 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. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | 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 |
收录类别 | SCI ; EI |
原文出处 | http://www.aanda.org/articles/aa/abs/2016/04/aa26077-15/aa26077-15.html |
语种 | 英语 |
WOS记录号 | WOS:000373207800100 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/9585] ![]() |
专题 | 云南天文台_大样本恒星演化研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
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. 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.(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). |
入库方式: OAI收割
来源:云南天文台
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