Gas-dust plasma in the envelopes of T Tauri stars

Details Gas-dust plasma in the envelopes of T Tauri stars Gas-dust plasma in the envelopes of T Tauri stars

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..517g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, July 1985, p. 517-523) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, July-Aug

Astronomy and Astrophysics

Astronomy

Binary Stars, Cosmic Dust, Cosmic Plasma, Infrared Astronomy, Stellar Envelopes, T Tauri Stars, Linear Polarization, Stellar Magnetic Fields, Stellar Orbits, Stokes Law Of Radiation

Scientific paper

A model binary system, with the infrared companion's radiation being scattered in the primary's optically thin ellipsoidal envelope, is adopted to analyze the infrared linear-polarization spectrum of RY Tau. This binary has a 3-yr orbital period. Both the wavelength dependence of the envelope flattening and the mismatch of the (Q, U) polarization vector with the orbital phase on certain dates are attributable to charged particles whose gyroradii have a large dispersion in the star's variable magnetic field.

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