The nature of the X-ray emission in the Be star 1H1249-637

Details The nature of the X-ray emission in the Be star 1H1249-637 The nature of the X-ray emission in the Be star 1H1249-637

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprn17059t&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

In this paper we give new insight into the nature of the X-ray emisssion of the Be/X-ray binary candidate 1H1249-637. The X-ray spectrum is more consistent with a white dwarf, rather than a neutron star, as the compact object. This challenges current theories since the primary is a B0.5III star. Otherwise, this object would belong to a new class of objects, hot stars whose X-ray emission is not connected with a compact companion.

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