Statistics – Computation
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...221...62p&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 221, no. 1, Aug. 1989, p. 62-64.
Statistics
Computation
1
Absorption Spectra, Astronomical Spectroscopy, Stellar Mass Accretion, X Ray Binaries, Companion Stars, Computational Astrophysics, Early Stars, Roche Limit, Tides
Scientific paper
The possibility that structures in the outer parts of accretion disks are produced by the tidal action of a secondary which is overflowing its Roche lobe is explored. In the present model, the structures at various phases (with mideclipse as the 0 phase) are formed due to the impact of inhomogeneous tidal forces on matter in the outer parts of the disk. It is pointed out that the effect is more pronounced at phases 0.2 and 0.8, with maxima occurring between phases 0.2 and 0.3 and between phases 0.7 and 0.8 where it is assumed that the outflowing matter (through the first Lagrangian point) meets the disk.
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