Twisted accretion discs. III - Application to Epsilon Aurigae

Details Twisted accretion discs. III - Application to Epsilon Aurigae Twisted accretion discs. III - Application to Epsilon Aurigae

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.225..823k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 225, April 15, 1987, p. 823-835. Research supported by

Astronomy and Astrophysics

Astronomy

11

Accretion Disks, Eclipsing Binary Stars, Light Curve, Stellar Mass Accretion, Companion Stars, Precession, Stellar Structure, Viscosity

Scientific paper

Twisting and alignment in a steady-state circumbinary accretion disc is
studied. It is then used to account for observed features in the
scenario of Epsilon Aurigae as a triple. The alignment depends on
viscosity in the disc, but it is always substantial and leads to a
tilted slab-like profile when viewed edge-on.

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