The Formation of Precessional Spiral Density Wave in Accretion Disks and a New Model for Superoutbursts in SU UMa-type Binaries

Details The Formation of Precessional Spiral Density Wave in Accretion Disks and a New Model for Superoutbursts in SU UMa-type Binaries The Formation of Precessional Spiral Density Wave in Accretion Disks and a New Model for Superoutbursts in SU UMa-type Binaries

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006chjas...6a.159b&link_type=abstract

Chinese Journal of Astronomy and Astrophysics, Supplement, Volume 6, Issue S1, pp. 159-163 (2006).

Astronomy and Astrophysics

Astrophysics

7

Scientific paper

The three-dimensional gas dynamic simulations in SU UMa-type binaries show the formation of the precessional spiral density wave in inner parts of the accretion disk that are not subjected to gas dynamic perturbations. The features of the precessional spiral wave can explain both the energy release in the superoutburst and appearance of a superhump on the orbital light curve.

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