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Merging of Iron Lines in Spectra of X-ray Burst Sources
Published online by Cambridge University Press: 12 April 2016
Abstract
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Model atmospheres and synthetic spectra of neutron star of the effective temperature 107 K are presented. All the iron spectral features in the energy range 6-10 keV (uncorrected for redshift) are washed out by instrumental or intrinsic broadening, which leaves only a single line of the equivalent width comparable with the observations.
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- 2. Magnetic Effects
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- Copyright © Cambridge University Press 1990
References
Griem, H.R.
1974, Spectral Line Broadening by Plasmas, Academic Press, New York and London.Google Scholar
Mewe, R., Gronenschild, E.H.B.M., and van den Oord, G.H.J. 1985, Astron. Astrophys. Suppl., 62, 197.Google Scholar
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