Nova Cygni 1975 - A mechanism for the postmaximum quasi-eclipses

Details Nova Cygni 1975 - A mechanism for the postmaximum quasi-eclipses Nova Cygni 1975 - A mechanism for the postmaximum quasi-eclipses

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978sval....4..141i&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, June 1978, p. 260-265.) Soviet Astronomy Letters, vol. 4, May-June 1978, p. 141-144.

Astronomy and Astrophysics

Astronomy

2

Novae, Photosphere, Solar Eclipses, Stellar Envelopes, Stellar Mass Ejection, Binary Stars, Dwarf Stars, Planetary Rotation, Stellar Models

Scientific paper

The outflow of gas in the extended envelope of Nova Cygni 1975 followed a spiral pattern, so that the geometry of the effective photosphere differs from a figure of revolution. The apparent rotation of this nonaxisymmetric photosphere induces periodic light variations whose period is independent of the size of the photosphere but is sensitive to changes in the density and velocity of the ejected material.

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