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The core-degenerate scenario for the progenitors of Type Ia supernovae
Wang B(王博)1,2,3; Zhou, W. -H.2,4; Zuo, Z. -Y.5; Li, Y. -B.6; Luo, X.7; Zhang JJ(张居甲)1,2; Liu DD(刘栋栋)1,2,3; Wu CY(吴程远)1,2,3
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2017-02-01
Volume464Issue:4Pages:3965-3971
DOI10.1093/mnras/stw2646
Contribution Rank第1完成单位
Indexed BySCI
KeywordBinaries: Close Stars: Evolution Supernovae: General White Dwarfs
Abstract

The origin of the progenitors of Type Ia supernovae (SNe Ia) is still uncertain. The core-degenerate (CD) scenario has been proposed as an alternative way for the production of SNe Ia. In this scenario, SNe Ia are formed at the final stage of common-envelope evolution from a merger of a carbon-oxygen white dwarf (CO WD) with the CO core of an asymptotic giant branch companion. However, the birthrates of SNe Ia from this scenario are still not well determined. In this work, we performed a detailed investigation on the CD scenario based on a binary population synthesis approach. The SN Ia delay times from this scenario are basically in the range of 90-2500 Myr, mainly contributing to the observed SNe Ia with short and intermediate delay times, although this scenario can also produce some old SNe Ia. Meanwhile, our work indicates that the Galactic birthrates of SNe Ia from this scenario are not more than 20 per cent of total SNe Ia due to more careful treatment of mass transfer. Although the SN Ia birthrates in this work are lower than those in Ilkov & Soker, the CD scenario cannot be ruled out as a viable mechanism for the formation of SNe Ia. Especially, SNe Ia with circumstellar material from this scenario contribute to 0.7-10 per cent of total SNe Ia, which means that the CD scenario can reproduce the observed birthrates of SNe Ia like PTF 11kx. We also found that SNe Ia happen systemically earlier for a high value of metallicity and their birthrates increase with metallicity.

Funding ProjectNational Basic Research Program of China (973 programme)[2014CB845700] ; National Natural Science Foundation of China[11673059] ; National Natural Science Foundation of China[11322327] ; National Natural Science Foundation of China[11390374] ; National Natural Science Foundation of China[11521303] ; National Natural Science Foundation of China[11303036] ; National Natural Science Foundation of China[11573021] ; National Natural Science Foundation of China[11403096] ; National Natural Science Foundation of China[61561053] ; Chinese Academy of Sciences[QYZDB-SSW-SYS001] ; Chinese Academy of Sciences[XDB09010202] ; Chinese Academy of Sciences[KJZD-EW-M06-01] ; Fundamental Research Funds for the Central Universities ; Natural Science Basic Research Program of Shaanxi Province - Youth Talent Project[2016JQ1016] ; Natural Science Foundation of Yunnan Province[2013HB097] ; Natural Science Foundation of Yunnan Province[2013FB083] ; Youth Innovation Promotion Association CAS
Funding OrganizationNational Basic Research Program of China (973 programme)[2014CB845700] ; National Natural Science Foundation of China[11673059, 11322327, 11390374, 11521303, 11303036, 11573021, 11403096, 61561053] ; Chinese Academy of Sciences[QYZDB-SSW-SYS001, XDB09010202, KJZD-EW-M06-01] ; Fundamental Research Funds for the Central Universities ; Natural Science Basic Research Program of Shaanxi Province - Youth Talent Project[2016JQ1016] ; Natural Science Foundation of Yunnan Province[2013HB097, 2013FB083] ; Youth Innovation Promotion Association CAS
Language英语
Subject Area天文学 ; 恒星与银河系 ; 恒星物理学 ; 恒星形成与演化
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherOXFORD UNIV PRESS
Publication PlaceGREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
ISSN0035-8711
URL查看原文
Archive Date2017-01-10
WOS IDWOS:000393780500014
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordDELAY-TIME DISTRIBUTION ; WHITE-DWARF BINARIES ; MASS-RATIO DISTRIBUTION ; STAR DONOR CHANNEL ; COMMON ENVELOPE ; DIFFERENT METALLICITIES ; SPECTROSCOPIC BINARIES ; POPULATION SYNTHESIS ; PLANETARY-NEBULAE ; PTF 11KX
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9982
Collection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
Corresponding AuthorWang B(王博)
Affiliation1.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.Yunnan Minzu University, Kunming 650031, China
5.School of Science, Xi’an Jiaotong University, Xi’an 710049, China
6.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
7.Department of Astronomy, Beijing Normal University, Beijing 100875, China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Wang B,Zhou, W. -H.,Zuo, Z. -Y.,et al. The core-degenerate scenario for the progenitors of Type Ia supernovae[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,464(4):3965-3971.
APA Wang B.,Zhou, W. -H..,Zuo, Z. -Y..,Li, Y. -B..,Luo, X..,...&Wu CY.(2017).The core-degenerate scenario for the progenitors of Type Ia supernovae.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,464(4),3965-3971.
MLA Wang B,et al."The core-degenerate scenario for the progenitors of Type Ia supernovae".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 464.4(2017):3965-3971.
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