Possible existence of spectral lines in the soft X-ray or far ultraviolet region in HER X-1

Details Possible existence of spectral lines in the soft X-ray or far ultraviolet region in HER X-1 Possible existence of spectral lines in the soft X-ray or far ultraviolet region in HER X-1

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982acaps...2...71l&link_type=abstract

(Acta Astrophysica Sinica, vol. 2, no. 1, 1982, p. 71-73.) Chinese Astronomy and Astrophysics, vol. 6, Mar. 1982, p. 90, 91. Tra

Astronomy and Astrophysics

Astrophysics

Binary Stars, Line Spectra, Stellar Spectra, X Ray Sources, Electron Cyclotron Heating, Electron Density (Concentration), Far Ultraviolet Radiation, Landau Factor, Relativistic Electron Beams, Stellar Magnetic Fields

Scientific paper

It is shown that some lines in the soft X-ray or far UV region in Her X-1 can be predicted if the electron anomalous magnetic moment is taken into account. These lines are produced by the spin flipover of electrons near the Landau energy levels in a magnetic field with a value of 67 eV if nonrelativistic and a value of several hundred eV if relativistic. A calculation of intensity shows that, allowing for coherency, these lines may be observable.

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