On the Population of Wind-Accreting Neutron Stars in the Galaxy

On the Population of Wind-Accreting Neutron Stars in the Galaxy

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We explore the possibility that neutron stars accreting from the winds of main-sequence stellar companions account for a significant fraction of low-luminosity, hard X-ray sources (L_X <~ 10^35 ergs/s; 1-10 keV) in the Galaxy. This work was motivated by recent Chandra observations of the Gala...

書誌詳細
主要な著者:	Pfahl, E, Rappaport, S, Podsiadlowski, P
フォーマット:	Journal article
出版事項:	2002

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