Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...357.1151s&link_type=abstract
Astronomy and Astrophysics, v.357, p.1151-1156 (2000)
Astronomy and Astrophysics
Astrophysics
5
Polarization, Scattering, Stars: Mass-Loss, Stars: Magnetic Fields
Scientific paper
We consider the single scattering of nonpolarized radiation of central star on the electrons of plasma outflow (stellar wind). We assume that such stellar wind is magnetized. It is shown that the scattered radiation acquires the integral linear polarization due to nonhomogeneous distribution of the Faraday rotation angles even for spherical stellar winds. For nonspherical winds, Faraday's rotation changes the spectrum of integral polarization drastically compared with the nonmagnetized case. The numerical calculations of the polarization spectra are presented for Parker's spherical model of magnetized stellar wind. Such spectra allow us to estimate the values of magnetic field and electron number density in stellar winds.
Gnedin Yu N.
Krymski Sh. T.
Silant'ev N. A.
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