Surface Hydrogen-burning Modeling of Supersoft X-Ray Binaries: Are They Type Ia Supernova Progenitors?-Reference-Cited by-同舟云学术

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Surface Hydrogen-burning Modeling of Supersoft X-Ray Binaries: Are They Type Ia Supernova Progenitors?

Published:2004-08-03 Issue:1 Volume:612 Page:L53-L56
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Starrfield S.,Timmes F. X.,Hix W. R.,Sion E. M.,Sparks W. M.,Dwyer S. J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference39 articles.

1. In Search of the Progenitors of Type IA Supernovae

2. CAL 87 - an eclipsing black hole binary?

3. Six Supersoft X‐Ray Binaries: System Parameters and Twin‐Jet Outflows

4. OPTICAL SPECTRA OF SUPERNOVAE

5. A theory of hydrogen shell flashes on accreting white dwarfs. I - Their progress and the expansion of the envelope. II - The stable shell burning and the recurrence period of shell flashes

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1. A soft and transient ultraluminous X-ray source with six-hour modulation in the NGC\,300 galaxy;Astronomy & Astrophysics;2023-12-14

2. Revised ephemeris and orbital period derivative of the supersoft X-ray source CAL 87 based on 34 yr of observations;Monthly Notices of the Royal Astronomical Society;2023-11-27

3. The 2019 Outburst of the 2005 Classical Nova V1047 Cen: A Record Breaking Dwarf Nova Outburst or a New Phenomenon?;The Astrophysical Journal;2022-10-26

4. Optical and near-infrared data and modelling of nova V5668 Sgr;Monthly Notices of the Royal Astronomical Society;2022-01-14

5. Discovery of an ∼30-yr-duration post-nova pulsating supersoft source in the Large Magellanic Cloud;Monthly Notices of the Royal Astronomical Society;2020-09-24

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