Off-centre carbon burning in He-accreting carbon-oxygen white dwarfs | |
Wu CY(吴程远)1,2,3; Wang B(王博)1,2,3 | |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
2019-07-01 | |
卷号 | 486期号:3页码:2977-2981 |
关键词 | binaries: close stars: evolution supernovae: general white dwarfs |
ISSN号 | 0035-8711 |
DOI | 10.1093/mnras/stz1028 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | The carbon-oxygen white dwarf (CO WD) + He star channel is one of the promising ways for producing type Ia supernovae (SNe Ia) with short delay times. Recent studies found that carbon under the He shell can be ignited if the mass-accretion rate of CO WD is higher than a critical rate (about 2 x 10(-6)M(circle dot) yr(-1)), triggering an inwardly propagating carbon flame. Previous studies usually supposed that the off-centre carbon flame would reach the centre, resulting in the formation of an oxygen-neon (ONe) WD that will collapse into a neutron star. However, the process of off-centre carbon burning is not well studied. This may result in some uncertainties on the final fates of CO WDs. By employing MESA, we simulated the long-term evolution of off-centre carbon burning in He-accreting CO WDs. We found that the inwardly propagating carbon flame transforms the CO WDs into OSi cores directly but not ONe cores owing to the high temperature of the burning front. We suggest that the final fates of the CO WDs may be OSi WDs under the conditions of off-centre carbon burning, or explode as iron-core-collapse SNe if the mass accretion continues. We also found that the mass fractions of silicon in the OSi cores are sensitive to the mass-accretion rates. |
学科主题 | 天文学 ; 恒星与银河系 ; 恒星物理学 ; 恒星形成与演化 |
URL标识 | 查看原文 |
出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
资助项目 | National Natural Science Foundation of China[11873085] ; National Natural Science Foundation of China[11673059] ; National Natural Science Foundation of China[11521303] ; Chinese Academy of Sciences[KJZD-EW-M06-01] ; Chinese Academy of Sciences[QYZDB-SSW-SYS001] ; Natural Science Foundation of Yunnan Province[2018FB005] ; Natural Science Foundation of Yunnan Province[2017HC018] |
WOS关键词 | PROGENITORS ; SUPERNOVAE ; EVOLUTION ; BINARIES ; SYSTEMS ; CHANNEL ; MODEL |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000474903500001 |
资助机构 | National Natural Science Foundation of China[11873085, 11673059, 11521303] ; Chinese Academy of Sciences[KJZD-EW-M06-01, QYZDB-SSW-SYS001] ; Natural Science Foundation of Yunnan Province[2018FB005, 2017HC018] |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/20572] |
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); Wang B(王博) |
作者单位 | 1.Key Laboratory for the Structure and Evolution of Celestial Objects, Yunnan Observatories, CAS, Kunming 650216, China 2.University of Chinese Academy of Sciences, Beijing 100049, China 3.Centre for Astronomical Mega-Science, CAS, Beijing 100012, China |
推荐引用方式 GB/T 7714 | Wu CY,Wang B. Off-centre carbon burning in He-accreting carbon-oxygen white dwarfs[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,486(3):2977-2981. |
APA | Wu CY,&Wang B.(2019).Off-centre carbon burning in He-accreting carbon-oxygen white dwarfs.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,486(3),2977-2981. |
MLA | Wu CY,et al."Off-centre carbon burning in He-accreting carbon-oxygen white dwarfs".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 486.3(2019):2977-2981. |
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