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    Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/38650


    Title: Does the iron K alpha line of active galactic nuclei arise from the Cerenkov line-like radiation?
    Authors: You,JH;Liu,DB;Chen,WP;Chen,L;Zhang,SN
    Contributors: 物理研究所
    Keywords: 1 GALAXY MCG-6-30-15;GAMMA-RAY BURSTS;THIN CLOUDS;CENTRAL REGIONS;ACCRETION DISK;XMM-NEWTON;VARIABILITY;CONSTRAINTS;EMISSION;MODEL
    Date: 2003
    Issue Date: 2010-07-08 13:34:07 (UTC+8)
    Publisher: 中央大學
    Abstract: When thermal relativistic electrons with isotropic distribution of velocities move in a gas region or impinge upon the surface of a cloud that consists of a dense gas or doped dusts, the Cerenkov effect produces peculiar atomic or ionic emission lines, wh
    Relation: ASTROPHYSICAL JOURNAL
    Appears in Collections:[物理研究所] 期刊論文

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