| Accretion by a Neutron Star Moving at a High Kick Velocity in the Supernova Ejecta |
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| 作者姓名： | Xu Zhang Ye Lu and Yong-Heng Zhao National Astronomical Observatories Chinese Academy of Sciences Beijing |
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| 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 |
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| 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) |
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| 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…
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| 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 |
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| Xu Zhang,,Ye Lu, and Yong-Heng Zhao National Astronomical Observatories,Chinese Academy of Sciences,Beijing , .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. |
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| Authors: | Xu Zhang Ye Lu Yong-Heng Zhao |
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| Institution: | [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 |
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| Abstract: | |
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| Keywords: | pulsars: general-pulsars - stars: neutron - X-rays: stars - accretion diskinstability |
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