The accretion disk in NGC 4258

Details The accretion disk in NGC 4258 The accretion disk in NGC 4258

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..431..285h&link_type=abstract

Accretion processes in astrophysical systems: Some like it hot! - eigth astrophysics conference. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astrophysics

Infall, Accretion, And Accretion Disks, Interstellar Masers, Active And Peculiar Galaxies And Related Systems

Scientific paper

In the framework of α-disk models, we show that the accretion disk in NGC 4258 is self-gravitating at the distance where the masing regions are observed, whatever the accretion rate. This conclusion holds in the presence of the external irradiation. As a result, the maser region cannot involve the whole disk thickness as proposed by Neufeld & Maloney (1995).

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