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Does the Radiative Avalanche Fueling Work in Any Active Galactic Nuclei?
Author(s) -
Yoshiaki Taniguchi
Publication year - 1997
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/310864
Subject(s) - physics , radiative transfer , active galactic nucleus , accretion (finance) , astrophysics , radiation , astronomy , galaxy , nuclear physics , optics
Recently Umemura, Fukue, & Mineshige (1997) proposed the radiative avalanchefueling to active galactic nuclei; gas accretion is driven by radiation dragexerted by stellar radiation from circumnuclear starburst regions. Thismechanism is also interesting in terms of starburst-AGN connections. Wetherefore present observational tests for the radiative avalanche fueling. Ourtests, however, show that gas accretion rates driven by the radiative avalancheare significantly lower than those expected from the standard accretion theoryapplied for typical active galactic nuclei with the circumnuclear starburstregions. Instead we propose an alternative, possible starburst-AGN connection;a minor merger with a nucleated satellite drives circumnuclear starbursts andthen leads to gas fueling onto the central engine as the merger proceeds.Comment: 12 page

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