On the source of optical variability and outflow in the Z CMa system

Details On the source of optical variability and outflow in the Z CMa system On the source of optical variability and outflow in the Z CMa system

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arep...42..630l&link_type=abstract

Astronomy Reports, Volume 42, Issue 5, September 1998, pp.630-637

Astronomy and Astrophysics

Astronomy

4

Scientific paper

It is proposed that the main source of stellar wind and optical variability in the binary system Z CMa is the optical primary, rather than its so-called infrared companion. The higher polarization of the spectral lines compared to the continuum is interpreted as the result of Thomson scattering of the line radiation in the region where it forms, i.e., in the stellar wind.

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