Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae
文献类型:期刊论文
作者 | Wu CY(吴程远)1,2,3,4; Wang B(王博)1,2,3,4; Liu DD(刘栋栋)1,2,3,4; Han ZW(韩占文)1,2,3,4 |
刊名 | ASTRONOMY & ASTROPHYSICS |
出版日期 | 2017-08-01 |
卷号 | 604 |
ISSN号 | 0004-6361 |
关键词 | Stars: Evolution Binaries (Including Multiple): Close Supernovae: General White Dwarfs |
DOI | 10.1051/0004-6361/201630099 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | Context. Type Ia supernovae (SNe Ia) play a crucial role in studying cosmology and galactic chemical evolution. They are thought to be thermonuclear explosions of carbon-oxygen white dwarfs (CO WDs) when their masses reach the Chandrasekar mass limit in binaries. Previous studies have suggested that He novae may be progenitor candidates of SNe Ia. However, the mass retention efficiencies during He nova outbursts are still uncertain. |
学科主题 | 天文学 ; 恒星与银河系 ; 恒星物理学 |
URL标识 | 查看原文 |
出版地 | 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE |
WOS关键词 | SINGLE-DEGENERATE CHANNEL ; EDDINGTON WIND SCENARIO ; AM CVN STARS ; LIGHT CURVES ; HELIUM NOVA ; SHELL SOURCE ; DELAY TIMES ; PROGENITORS ; EVOLUTION ; BINARIES |
资助项目 | National Basic Research Program of China (973 programme)[2014CB845700] ; National Natural Science Foundation of China[11673059] ; National Natural Science Foundation of China[11521303] ; National Natural Science Foundation of China[11390374] ; National Natural Science Foundation of China[11573016] ; National Natural Science Foundation of China[11573016] ; Chinese Academy of Sciences[KJZD-EW-M06-01] ; Key Research Program of Frontier Science CAS[QYZDB-SSW-SYS001] ; Youth Innovation Promotion Association CAS ; Natural Science Foundation of Yunnan Province[2013HB097] ; Natural Science Foundation of Yunnan Province[2013HA005] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | EDP SCIENCES S A |
WOS记录号 | WOS:000408480100038 |
资助机构 | National Basic Research Program of China (973 programme)[2014CB845700] ; National Natural Science Foundation of China[11673059, 11521303, 11390374, 11573016, 11547041] ; Chinese Academy of Sciences[KJZD-EW-M06-01] ; Key Research Program of Frontier Science CAS[QYZDB-SSW-SYS001] ; Youth Innovation Promotion Association CAS ; Natural Science Foundation of Yunnan Province[2013HB097, 2013HA005] |
源URL | [http://ir.ynao.ac.cn/handle/114a53/10164] |
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 |
通讯作者 | Wu CY(吴程远) |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming; 650216, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming; 650216, China 3.University of Chinese Academy of Sciences, Beijing; 100049, China 4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing; 100012, China |
推荐引用方式 GB/T 7714 | Wu CY,Wang B,Liu DD,et al. Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae[J]. ASTRONOMY & ASTROPHYSICS,2017,604. |
APA | Wu CY,Wang B,Liu DD,&Han ZW.(2017).Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae.ASTRONOMY & ASTROPHYSICS,604. |
MLA | Wu CY,et al."Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae".ASTRONOMY & ASTROPHYSICS 604(2017). |
入库方式: OAI收割
来源:云南天文台
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