AbstractStrange stars with low masses are suggested to exist in reality, the origin of which could be via accretion-induced collapse of white dwarfs. Such a strange star is likely bare, and would thus spin very fast, even to a period of <0.1ms. Strange stars with low masses may differ from those with solar masses in various astrophysical appearances. Observations to test this “low-mass” idea are proposed.


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    Titel :

    Low-mass bare strange stars


    Beteiligte:
    Xu, R.X. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 37 , 10 ; 1992-1995


    Erscheinungsdatum :

    2005-10-17


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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