Abstract This paper gives decription of computer code for model atmosphere and line profile computations of X-ray burst sources, with theoretical models and predicted equivalent widths WE of resonance lines of iron (H-like and He-like ions). The models show, that iron lines are very strong in atmospheres of neutron stars at effective temperature Te = 107K, and should exhibit WE approaching hundreds of eV.
Model computations of iron absorption lines in X-ray burst spectra
Advances in Space Research ; 8 , 2-3 ; 481-484
1988-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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