Evolution of long-period, white-dwarf binaries: application to GRO J1744-28 and type Ia supernovae-Reference-Cited by-同舟云学术

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Evolution of long-period, white-dwarf binaries: application to GRO J1744-28 and type Ia supernovae

Published:2009-01-14 Issue:1 Volume:495 Page:243-248
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Xu Xiao-Jie,Li Xiang-Dong

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:200810238/pdf

Reference52 articles.

1. Low-temperature Rosseland opacities

2. Cataclysmic Variables: An Empirical Angular Momentum Loss Prescription from Open Cluster Data

3. Evolving to Type Ia Supernovae with Long Delay Times

4. Evidence for “Propeller” Effects in X-Ray Pulsars GX 1+4 and GRO J1744−28

5. The ExtendedHSTSupernova Survey: The Rate of SNe Ia atz> 1.4 Remains Low

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1. The Progenitors of Type Ia Supernovae with Asymptotic Giant Branch Donors;Research in Astronomy and Astrophysics;2023-06-15

2. White dwarf mass growth in cataclysmic variables: roles of dwarf novae;Monthly Notices of the Royal Astronomical Society;2023-05-15

3. The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries;Research in Astronomy and Astrophysics;2020-09-01

4. A strange star scenario for the formation of isolated millisecond pulsars;Astronomy & Astrophysics;2020-01

5. Mass-accreting white dwarfs and type Ia supernovae;Research in Astronomy and Astrophysics;2018-05

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