ar X iv : a st ro - p h / 96 04 18 3 v 1 3 0 A pr 1 99 6 Counter - Rotating Accretion Disks
نویسنده
چکیده
We consider accretion disks consisting of counter-rotating gaseous components with an intervening shear layer. Configurations of this type may arise from the accretion of newly supplied counter-rotating gas onto an existing co-rotating gas disk. For simplicity we consider the case where the gas well above the disk midplane is rotating with angular rate +Ω and that well below has the same properties but is rotating with rate−Ω. Using the Shakura-Sunyaev alpha turbulence model, we find self-similar solutions where a thin (relative to the full disk thickness) equatorial layer accretes very rapidly, essentially at free-fall speed. As a result the accretion speed is much larger than it would be for an alpha disk rotating in one direction. Counter-rotating accretion disks may be a transient stage in the formation of counter-rotating galaxies and in the accretion of matter onto compact objects. Subject headings: accretion disks counter-rotating galaxies
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