Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-03-17
Astronomy and Astrophysics
Astrophysics
submitted to ApJ Letters
Scientific paper
10.1086/341197
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 Galactic center by Wang et al. (2002). Our calculations indicate that many of the discrete X-ray sources detected in this survey may be wind-accreting neutron stars, and that many more may be discovered with deeper X-ray observations. We propose that an infrared observing campaign be undertaken to search for the stellar counterparts of these X-ray sources.
Pfahl Eric
Podsiadlowski Ph
Rappaport Saul
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