X-ray emission from single magnetic early-type stars

Details X-ray emission from single magnetic early-type stars X-ray emission from single magnetic early-type stars

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...395..575u&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 395, no. 2, Aug. 20, 1992, p. 575-581.

Astronomy and Astrophysics

Astrophysics

40

Bremsstrahlung, Early Stars, Stellar Luminosity, Stellar Magnetic Fields, X Ray Stars, Current Sheets, Gas Heating, Stellar Magnetospheres, Stellar Rotation, Wolf-Rayet Stars

Scientific paper

A new model for the X-ray emission from single early-type stars is presented. X-rays observed from these stars can be produced by the hot gas near the current sheet via the bremsstrahlung mechanism. Gas heating in the current sheet is considered and the X-ray luminosity of single magnetic early-type stars is estimated. Theoretical predictions of the model about the properties of X-rays are discussed.

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