Intrinsic polarization in Beta Lyrae and Nova T-Pyxidis due to irradiation of silicate glassy grains

Details Intrinsic polarization in Beta Lyrae and Nova T-Pyxidis due to irradiation of silicate glassy grains Intrinsic polarization in Beta Lyrae and Nova T-Pyxidis due to irradiation of silicate glassy grains

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..93..347s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 93, no. 2, June 1983, p. 347-349.

Astronomy and Astrophysics

Astronomy

1

Eclipsing Binary Stars, Novae, Polarization Characteristics, Silicates, Stellar Envelopes, Ultraviolet Astronomy, X Ray Sources, Electron Irradiation, Interstellar Extinction, Stellar Flares, X Ray Irradiation

Scientific paper

The intrinsic polarization in the binary system Beta Lyrae and in Nova T-Pyxidis probably has X- and/or UV-irradiation of silicate glass-like grains as the main governing mechanism. The objects studied possess extended atmospheres showing strong evidence for condensation processes that produce solid particles. The origin of the flaring mechanism may be different in different types of stars, but the accompanying energetic radiation is common.

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