Radiative Avalanche Driven by Spherical Starbursts

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We examine a radiative avalanche for the case of spherically distributed sources. A radiative avalanche is a new mechanism, in which the mass-accretion of the nuclear disk is driven via radiation drag exerted by stellar radiation from circumnuclear starburstregions, and which is expected to be a link between starburst activities and AGNs. The results of the present spherical case are qualitatively similar to those of the ringlike case. However, the solid angle subtended by the starburst region is large and the radiation field of the starburst region has no angular momentum, which are in favor for the avalanche model. In addition, an avalanche can take place continuously from the outside to the inside of the starburst region in the spherical case.

収録刊行物

  • PASJ : publications of the Astronomical Society of Japan

    PASJ : publications of the Astronomical Society of Japan 49(6), 673-677, 1997-12-01

    Astronomical Society of Japan

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各種コード

  • NII論文ID(NAID)
    10002598844
  • NII書誌ID(NCID)
    AA1082896X
  • 本文言語コード
    ENG
  • 資料種別
    ART
  • ISSN
    00046264
  • NDL 記事登録ID
    4384250
  • NDL 雑誌分類
    ZM33(科学技術--宇宙科学)
  • NDL 請求記号
    Z53-A296
  • データ提供元
    CJP書誌  NDL  IR 
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