Off-centre carbon burning in He-accreting carbon–oxygen white dwarfs-Reference-Cited by-同舟云学术

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Off-centre carbon burning in He-accreting carbon–oxygen white dwarfs

Published:2019-04-12 Issue:3 Volume:486 Page:2977-2981
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Wu Chengyuan¹²³,Wang Bo¹²³^ORCID

Affiliation:

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

Funder

National Natural Science Foundation of China

Chinese Academy of Sciences

Natural Science Foundation of Yunnan Province

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1028/28369980/stz1028.pdf

Reference46 articles.

1. CARBON SHELL OR CORE IGNITIONS IN WHITE DWARFS ACCRETING FROM HELIUM STARS

2. Accretion-induced Collapse from Helium Star + White Dwarf Binaries

3. HD 49798: Its History of Binary Interaction and Future Evolution

4. MESA MODELS OF CLASSICAL NOVA OUTBURSTS: THE MULTICYCLE EVOLUTION AND EFFECTS OF CONVECTIVE BOUNDARY MIXING

Cited by 10 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Evolution of double oxygen–neon white dwarf merger remnant;Monthly Notices of the Royal Astronomical Society;2023-09-07

2. Detector induced anisotropies on the angular distribution of gravitational wave sources and opportunities of constraining horizon scale anisotropies;Monthly Notices of the Royal Astronomical Society;2023-08-31

3. Evolution of Carbon-Oxygen White Dwarf Accreting Helium as One of the Progenitors of Accretion-induced Collapse;Journal of Physics: Conference Series;2022-11-01

4. X-ray pulsar HD 49798: a contracting white dwarf with a debris disk?;Astronomy & Astrophysics;2022-06

5. Formation of ultra-massive carbon–oxygen white dwarfs from the merger of carbon–oxygen and helium white dwarf pairs;Monthly Notices of the Royal Astronomical Society;2022-03-31

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