Abstract The decrease of the surface temperature TS and the increase of the fluid layer and convective region from the pole to the equator due to rapid rotation is calculated, taking into account several equations of state in the high-density region of the neutron star.


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    Title :

    On the structure of envelopes of rapidly rotating neutron stars


    Contributors:

    Published in:

    Advances in Space Research ; 8 , 2-3 ; 711-714


    Publication date :

    1988-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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