Discovery of a compact companion to the hot subdwarf star BD+37 442

We report the results of the first X-ray observation of the luminous and helium-rich O-type subdwarf BD+37 442, carried out with the XMM-Newton satellite in August 2011. X-ray emission is detected with a flux of about 3x10^(-14) erg/cm2/s (0.2-1 keV) and a very soft spectrum, well fit by the sum of...

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Bibliographic Details
Published in:arXiv.org 2012-04
Main Authors: La Palombara, N, Mereghetti, S, Tiengo, A, Esposito, P
Format: Article
Language:English
Subjects:
Blackbody
Deposition
Emission
Helium
Neutron flux
Neutron stars
Stellar winds
Subdwarf stars
White dwarf stars
XMM (spacecraft)
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Summary:We report the results of the first X-ray observation of the luminous and helium-rich O-type subdwarf BD+37 442, carried out with the XMM-Newton satellite in August 2011. X-ray emission is detected with a flux of about 3x10^(-14) erg/cm2/s (0.2-1 keV) and a very soft spectrum, well fit by the sum of a blackbody with temperature kT_BB = 45^(+11)_(-9) eV and a power law with a poorly constrained photon index. Significant pulsations with a period of 19.2 s are detected, indicating that the X-ray emission originates in a white dwarf or neutron star companion, most likely powered by accretion from the wind of BD+37 442.
ISSN:2331-8422
DOI:10.48550/arxiv.1204.3519