On the Population of Wind-Accreting Neutron Stars in the Galaxy
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...
मुख्य लेखकों: | Pfahl, E, Rappaport, S, Podsiadlowski, P |
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स्वरूप: | Journal article |
प्रकाशित: |
2002
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समान संसाधन
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On the population of wind-accreting neutron stars in the Galaxy
द्वारा: Pfahl, E, और अन्य
प्रकाशित: (2002) -
A comprehensive study of neutron star retention in globular clusters
द्वारा: Pfahl, E, और अन्य
प्रकाशित: (2002) -
A comprehensive study of neutron star retention in globular clusters
द्वारा: Pfahl, E, और अन्य
प्रकाशित: (2002) -
A new class of high-mass X-ray binaries: Implications for core collapse and neutron star recoil
द्वारा: Pfahl, E, और अन्य
प्रकाशित: (2002) -
A new class of high-mass X-ray binaries: Implications for core collapse and neutron-star recoil
द्वारा: Pfahl, E, और अन्य
प्रकाशित: (2002)