Supersoft X-Ray Sources Identified with Be Binaries in the Magellanic Clouds

Author:

Cracco ValentinaORCID,Orio MarinaORCID,Ciroi StefanoORCID,Gallagher JayORCID,Kotulla RalfORCID,Romero-Colmenero EncarniORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 7 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. X-raying the ζ Tau binary system;Astronomy & Astrophysics;2024-08

2. Velocity monitoring of γ Cas stars reveals their binarity status;Monthly Notices of the Royal Astronomical Society;2022-01-03

3. Swift J011511.0-725611: discovery of a rare Be star/white dwarf binary system in the SMC;Monthly Notices of the Royal Astronomical Society;2021-09-15

4. The CO White Dwarf + Intermediate-mass/Massive Star Binary Evolution: Possible Merger Origins for Peculiar Type Ia and II Supernovae;Publications of the Astronomical Society of the Pacific;2021-07-01

5. Swift J004427.3−734801 – a probable Be/white dwarf system in the Small Magellanic Cloud;Monthly Notices of the Royal Astronomical Society: Letters;2020-06-12

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