Abstract A map of the galactic center region in the 1.8 MeV gamma-ray line from radioactive Al26 was derived from balloon flight data of the MPI Compton telescope. The image of the observed region of the sky is consistent with a point source origin at l = 1° ± 4°, b = −30 ± 4°. Diffuse emission models from unresolved candidate sources like supernovae, novae, Wolf-Rayet stars, and massive stars fit our data worse than a point source, but cannot be rejected definitely.


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    Titel :

    Map of the galactic center region in the 1.8 MeV 26Al gamma-ray line


    Beteiligte:
    Ballmoos, P.V. (Autor:in) / Diehl, R. (Autor:in) / Schönfelder, V. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.01.1986


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch





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