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.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    On the structure of envelopes of rapidly rotating neutron stars


    Beteiligte:
    Geppert, U. (Autor:in) / Wiebicke, H.-J. (Autor:in)

    Erschienen in:

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


    Erscheinungsdatum :

    01.01.1988


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    Relativistic MHD winds from rotating neutron stars

    Bucciantini, N. | Online Contents | 2007


    On the possible existence of localised vacillating convection state in rapidly rotating young solar-like stars

    Ballot, J. / Brun, A. S. / Turck-Chieze, S. et al. | British Library Conference Proceedings | 2006



    NEUTRON STARS

    Online Contents | 1997


    Compact Circumstellar Dust Envelopes of Evolved AGB Stars with Heavy Mass Loss

    Hashimoto, O. / Izumiura, H. / International Council of Scientific Unions | British Library Conference Proceedings | 2000