Gravitational Instability of Rotating Viscoelastic Partially Ionized Plasma in the Presence of an Oblique Magnetic Field and Hall Current
Figure 2
Variation of , given by (14), with the wavenumber for different values of viscoelasticity when mHโcmโ1, โgmโcmโ1โsecโ1, โsecโ1, โradโsecโ1, โAmpโcmโ1, โgmโcmโ3, cm2โsecโ1, and .