On the Instability of the Collision Accretion Disk

Details On the Instability of the Collision Accretion Disk On the Instability of the Collision Accretion Disk

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pkas...12..149y&link_type=abstract

Publications of the Korean Astronomical Society, vol.12, no.1, p.149-157

Astronomy and Astrophysics

Astronomy

Scientific paper

The collision model of the disk, based on collisions between the particles in the disk, is summarized. The dependence of disk stability on the collision of the particles is demonstrated. The energy spectrum produced in the disk is numerically calculated. We concluded that the result are not largely different from those of the standard disk model. It implies that the collision of the particles inside the disk may be considered here.

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