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    Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/39215


    Title: CAN COSMIC-RAYS DOMINATE SUPERNOVA REMNANT SHOCKS
    Authors: KO,CM
    Contributors: 物理研究所
    Keywords: PARTICLE-ACCELERATION
    Date: 1995
    Issue Date: 2010-07-08 14:08:34 (UTC+8)
    Publisher: 中央大學
    Abstract: In this article we discuss the possibility of a cosmic-ray-dominated supernova remnant shock from the point of view of the diffusive confinement of cosmic rays near the shock. We examine the conditions under which this may be possible. Several examples are presented to illustrate the conditions. As expected, a cosmic-ray-dominated supernova remnant shock forms more 'easily' if the supernova progenitor has created a large wind bubble.
    Relation: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
    Appears in Collections:[物理研究所] 期刊論文

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