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Accretion by a Neutron Star Moving at a High Kick Velocity in the Supernova Ejecta
引用本文:Xu Zhang1,2,Ye Lu1,3 and Yong-Heng Zhao1 1 National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012, 2 Department of Physics,Shandong University,Jinan 250100 3 Department of Physics,The University of Hong Kong,Pokfulam Road,Hong Kong. Accretion by a Neutron Star Moving at a High Kick Velocity in the Supernova Ejecta[J]. 中国天文和天体物理学报, 2007, 7(1): 91-100
作者姓名:Xu Zhang1  2  Ye Lu1  3 and Yong-Heng Zhao1 1 National Astronomical Observatories  Chinese Academy of Sciences  Beijing 100012   2 Department of Physics  Shandong University  Jinan 250100 3 Department of Physics  The University of Hong Kong  Pokfulam Road  Hong Kong
作者单位:Xu Zhang1,2,Ye Lu1,3 and Yong-Heng Zhao1 1 National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012; 2 Department of Physics,Shandong University,Jinan 250100 3 Department of Physics,The University of Hong Kong,Pokfulam Road,Hong Kong
基金项目:国家自然科学基金;国家重点基础研究发展计划(973计划)
摘    要:1 INTRODUCTION The classical problem of spherical accretion onto a compact object, e.g., a black hole or a neutron star (NS), has been studied by many authors. A hydrodynamical solution was presented by Bondi 1952, who showed that inside a certain capture…

关 键 词:pulsars: general-pulsars—stars: neutron—X-rays: stars—accretion disk—instability

Accretion by a Neutron Star Moving at a High Kick Velocity in the Supernova Ejecta
Xu Zhang,Ye Lu,Yong-Heng Zhao. Accretion by a Neutron Star Moving at a High Kick Velocity in the Supernova Ejecta[J]. Chinese Journal of Astronomy and Astrophysics, 2007, 7(1): 91-100
Authors:Xu Zhang  Ye Lu  Yong-Heng Zhao
Affiliation:[1]National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 [2]Department of Physics, Shandong University, Jinan 250100 [3]Department of Physics, The University of Hong Kong, Pokfulam Road, Hong Kong
Abstract:
Keywords:pulsars: general-pulsars - stars: neutron - X-rays: stars - accretion diskinstability
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