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Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae
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
发表期刊ASTRONOMY & ASTROPHYSICS
2017-08-01
卷号604
DOI10.1051/0004-6361/201630099
产权排序第1完成单位
收录类别SCI ; EI
关键词Stars: Evolution Binaries (Including Multiple): Close Supernovae: General White Dwarfs
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.

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]
项目资助者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]
语种英语
学科领域天文学 ; 恒星与银河系 ; 恒星物理学
学科门类理学 ; 理学::天文学
文章类型Article
出版者EDP SCIENCES S A
出版地17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE
ISSN0004-6361
URL查看原文
WOS记录号WOS:000408480100038
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SINGLE-DEGENERATE CHANNEL ; EDDINGTON WIND SCENARIO ; AM CVN STARS ; LIGHT CURVES ; HELIUM NOVA ; SHELL SOURCE ; DELAY TIMES ; PROGENITORS ; EVOLUTION ; BINARIES
引用统计
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/10164
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).
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