The polarization of radiation from hot stars

Details The polarization of radiation from hot stars The polarization of radiation from hot stars

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..755l&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, July-Aug. 1987, p. 755-760. In Russian.

Statistics

Computation

Early Stars, Hot Stars, Polarization Characteristics, Stellar Radiation, Computational Astrophysics, Fourier Analysis, Stellar Atmospheres, Stellar Models

Scientific paper

The Feautrier method is used to calculate the degree of polarization of
radiation from hot stars. Model atmospheres of these stars which were
obtained by Kurucz (1979) are used. The results suggest that the natural
polarization of O and B stars is associated with the presence of
strongly nonspherical envelopes or accretion disks.

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