A new type of spiral waves in accretion discs

Details A new type of spiral waves in accretion discs A new type of spiral waves in accretion discs

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..330..383b&link_type=abstract

The Astrophysics of Cataclysmic Variables and Related Objects, Proceedings of ASP Conference Vol. 330. Edited by J.-M. Hameury a

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The possibility of formation of "precessional" spiral waves in binaries
with large mass ratios can be used to interpret observations of these
systems. There is no other reasonable explanation for the appearance of
superhumps at large mass ratios, so applications of the "precessional"
spiral wave model to binary systems like TV Col looks very promising.

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