Effects of spiral shocks on disk emission lines

Details Effects of spiral shocks on disk emission lines Effects of spiral shocks on disk emission lines

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...271..216c&link_type=abstract

Astronomy and Astrophysics, Vol. 271, p. 216 (1993)

Astronomy and Astrophysics

Astrophysics

20

Accretion, Be Stars, Cataclysmic Variables, Emission Lines

Scientific paper

We show that spiral shocks on stellar disks, induced by binary companions, can have significant effects upon observable emission lines. For an even number of shocks, the separations and heights of the two-horned emission lines will vary with binary phase, while for an odd number of shocks, red/blue asymmetries appear, with the red and the blue components alternating in brightness.

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