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.


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    Titel :

    Model computations of iron absorption lines in X-ray burst spectra


    Beteiligte:
    Madej, J. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 8 , 2-3 ; 481-484


    Erscheinungsdatum :

    1988-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



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