Gravitational Instability of Rotating Viscoelastic Partially Ionized Plasma in the Presence of an Oblique Magnetic Field and Hall Current
Figure 4
Variation of , given by (14), with the wavenumber for different values of when gm cm−1 sec−2, mH cm−1, sec−1, rad sec−1, Amp cm−1, gm cm−1 sec−1, cm2 sec−1 and .