X-ray emission from hot subdwarfs with compact companions

We review the X-ray observations of hot subdwarf stars. While no X-ray emission has been detected yet from binaries containing B-type subdwarfs, interesting results have been obtained in the case of the two luminous O-type subdwarfs HD 49798 and BD +37 442. Both of them are members of binary systems...

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Bibliographic Details
Published in:arXiv.org 2012-10
Main Authors: Mereghetti, Sandro, Nicola La Palombara, Esposito, Paolo, Tiengo, Andrea
Format: Article
Language:English
Subjects:
Binary stars
Deposition
Emission
Luminosity
Neutron stars
Neutrons
Stellar winds
Subdwarf stars
White dwarf stars
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Summary:We review the X-ray observations of hot subdwarf stars. While no X-ray emission has been detected yet from binaries containing B-type subdwarfs, interesting results have been obtained in the case of the two luminous O-type subdwarfs HD 49798 and BD +37 442. Both of them are members of binary systems in which the X-ray luminosity is powered by accretion onto a compact object: a rapidly spinning (13.2 s) and massive (1.28 M_sun) white dwarf in the case of HD 49798 and most likely a neutron star, spinning at 19.2 s, in the case of BD +37 442. Their study can shed light on the poorly known processes taking place during common envelope evolutionary phases and on the properties of wind mass loss from hot subdwarfs.
ISSN:2331-8422
DOI:10.48550/arxiv.1210.6058