Hydromagnetic Instabilities in Proto–Neutron Stars
نویسندگان
چکیده
منابع مشابه
Hydromagnetic instabilities in proto–neutron stars
The stability properties of newly born neutron stars, or proto–neutron stars (PNSs), are considered. We take into account dissipative processes, such as neutrino transport and viscosity, in the presence of a magnetic field. In order to find the regions of the star subject to different sorts of instability, we derive the general instability criteria and apply it to evolutionary models of PNSs. T...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2002
ISSN: 0004-637X,1538-4357
DOI: 10.1086/340899