A new class of high-mass X-ray binaries: Implications for core collapse and neutron-star recoil

A new class of high-mass X-ray binaries: Implications for core collapse and neutron-star recoil

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We investigate an interesting new class of high-mass X-ray binaries (HMXBs) with long orbital periods (Porb > 30 days) and low eccentricities (e ≲ 0.2). The orbital parameters suggest that the neutron stars in these systems did not receive a large impulse, or "kick," at the time of...

書誌詳細
主要な著者:	Pfahl, E, Rappaport, S, Podsiadlowski, P, Spruit, H
フォーマット:	Journal article
出版事項:	Institute of Physics 2002
主題:	supernovae: general X-rays: stars stars: neutron

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