Low T/|W| dynamical instability in differentially rotating stars: diagnosis with canonical angular momentum
Motoyuki SaijoLaboratoire de l'Univers et de ses Théories, Observatoire de Paris, F‐92195 Meudon Cedex, FranceS. YoshidaDepartment of Physics, University of Wisconsin Milwaukee, Milwaukee WI 53211, USA
2006en
ABI
Annotatsiya
Stars in nature are usually rotating and may be subject to non-axisymmetric rotational instabilities. An analytically exact treatment of these instabilities in linearized theory exists only for incompressible equilibrium fluids in Newtonian
Hali tarjima qilinmagan
Identifikatorlar
Iqtiboslar va manbalar
2 ta iqtibos0 ta foydalanilgan manba