On the Interpretation of Doppler Tomograms of Dwarf Nova Disks During Outbursts

Details On the Interpretation of Doppler Tomograms of Dwarf Nova Disks During Outbursts On the Interpretation of Doppler Tomograms of Dwarf Nova Disks During Outbursts

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aca....51..295s&link_type=abstract

Acta Astronomica, v.51, pp.295-302, (2001).

Astronomy and Astrophysics

Astronomy

18

Accretion, Accretion Disks, Shock Waves, Novae, Cataclysmic Variables, Stars: Individual: Ss Cyg, Ex Dra, U Gem, Ip Peg

Scientific paper

Simple model of the disk based on purely mechanical, restricted three-body approximation is already sufficient to explain the presence and shapes of the two arch-like structures observed in Doppler tomograms of dwarf nova disks during their outbursts. In particular, it explains their non-equal intensities (which could not be explained by the 2D hydrodynamic, spiral-wave models).

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