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Polarized radiation in magnetic white dwarfs

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/154786· OSTI ID:7338111
A model for magnetic white dwarfs is proposed which attributes the partially polarized light to synchrotron radiation. The source of the radiation is relativistic electrons trapped in the magnetosphere of a white dwarf. The white dwarf's magnetic field is assumed to be dipolar. The Stokes parameters for the synchrotron radiation are tabulated as a function of frequency, observer's orientation, and energy and spatial distribution of the relativistic electrons. The results of the synchrotron calculations are applied to the polarization observations of Grw+70degree8247 and DQ Herculis. This model can account for the major features of the polarized radiation coming from these two magnetic white dwarfs. The calculations predict for Grw+70degree8247 that the surface magnetic field is B/sub s/approximately-less-than4 x 10/sup 6/ gauss, that the incident viewing angle is 45degreeapproximately-less-thantheta/sub 0/approximately-less-than75degree, and that the electrons are trapped with nearly an isotropic distribution about the white dwarf. For DQ Herculis the surface magnetic field is B/sub s/approximately-less-than7 x 10/sup 6/ gauss and the trapped electrons are confined to a dislike region about the white dwarf. For both cases the density of electrons in the magnetosphere falls in the range of 10/sup 5/approximately-less-thannapproximately-less-than10/sup 7/ cm/sup -3/ with energies of about 4--35 MeV. (AIP)
Research Organization:
Department of Physics and Institute of Theoretical Science, University of Oregon
OSTI ID:
7338111
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 209:3; ISSN ASJOA
Country of Publication:
United States
Language:
English