Gravitational Instability of Rotating Viscoelastic Partially Ionized Plasma in the Presence of an Oblique Magnetic Field and Hall Current
Table 3
Variation of , given by (14), with the wavenumber for different values of . At gm cm−1 sec−2, gm cm−1 sec−1, mH cm−1, sec−1, cm2 sec−1, gm cm−3, , and Amp cm−1.