AbstractThe detection of a soft thermal X-ray component in the spectrum of a bright knot in the halo of the plerion G21.5-0.9 is reported. Using a collisional ionization equilibrium model for an hot optically thin plasma, a temperature of kT 0.12–0.24keV, a mass of 0.3–1.0M⊙ and a density of 1.6–6cm−3 is derived. The spectral analysis suggests a possible overabundance of Silicon with respect to the solar value in the knot; if this will be confirmed this object may be a clump of shocked ejecta.


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    Titel :

    Detection of thermal X-ray emission in the halo of the plerionic supernova remnant G21.5-0.9


    Beteiligte:
    Bocchino, F. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 35 , 6 ; 1003-1006


    Erscheinungsdatum :

    2005-01-13


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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