A common-envelope wind model for Type Ia supernovae – I. Binary evolution and birth rate-Reference-Cited by-同舟云学术

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A common-envelope wind model for Type Ia supernovae – I. Binary evolution and birth rate

Published:2017-05-12 Issue:4 Volume:469 Page:4763-4787
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Meng X.¹²³,Podsiadlowski Ph.⁴

Affiliation:

1. Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, PR China

2. Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650216 Kunming, PR China

3. Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, PR China

4. Department of Astronomy, Oxford University, Oxford OX1 3RH, UK

Funder

Natural Science Foundation of China

CAS

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/469/4/4763/17729261/stx1137.pdf

Reference194 articles.

1. Nearby Supernova Factory Observations of SN 2005gj: Another Type Ia Supernova in a Massive Circumstellar Envelope

2. Low-temperature Rosseland opacities

3. Type I supernovae. I - Analytic solutions for the early part of the light curve

4. Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants?

5. Improved Hubble Space Telescope proper motions for Tycho-G and other stars in the remnant of Tycho's Supernova 1572

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