Iron Lines in Superstrong Magnetic Fields

Details Iron Lines in Superstrong Magnetic Fields Iron Lines in Superstrong Magnetic Fields

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phrvl..46.1700r&link_type=abstract

Physical Review Letters, Volume 46, Issue 26, June 29, 1981, pp.1700-1703

Physics

16

Neutron Stars, X-Ray Spectra, Zeeman And Stark Effects, X-Ray

Scientific paper

The possibility of observing atomic lines in the x-ray spectra of strongly magnetized accreting neutron stars is discussed. For magnetic field strengths ranging from 1011-1014 G, both the energies and oscillator strengths of Fe XXVI lines are calculated quantitatively. These lines are expected to be highest in energy, and should dominate at source temperatures kT~10-30 keV.

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