Superhumps in Binary Systems and Their Connection to Precessional Spiral Density Waves

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Details

LaTeX, 12 pages, 6 figures; figure 3 was improved

Scientific paper

10.1134/S1063772906070031

We consider a mechanism for the formation of superhumps in the TV Col system,
based on the possible existence of a precessional spiral wave in the accretion
disk of the system. This mechanism can act in binaries with arbitrary
component-mass ratios, and our precessional spiral wave model can be applied to
explain observed superhumps of all types.

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