Gravitational Instability of Rotating Viscoelastic Partially Ionized Plasma in the Presence of an Oblique Magnetic Field and Hall Current
Table 1
Variation of , given by (14), with the wavenumber for different values of . At โgmโcmโ1โsecโ2, โgmโcmโ1โsecโ1, โmHโcmโ1, โsecโ1, โradโsecโ1, โgmโcmโ3, โcm2โsecโ1, and โAmpโcmโ1.