Numerical modelling of cold accretion discs in cataclysmic variables: the superhump phenomenon

Details Numerical modelling of cold accretion discs in cataclysmic variables: the superhump phenomenon Numerical modelling of cold accretion discs in cataclysmic variables: the superhump phenomenon

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007a%26at...26...47b&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 26, Issue 1, p.47-52

Astronomy and Astrophysics

Astrophysics

Scientific paper

The three-dimensional gas dynamic simulations of flow structure in
binaries show the formation of the precessional spiral density wave in
inner parts of a cold accretion disc. The precessional wave model is
able to explain all types of observed superhump.

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