Effect of Radiative Heat-Loss Function and Finite Larmor Radius Corrections on Jeans Instability of Viscous Thermally Conducting Self-Gravitating Astrophysical Plasma

Figure 3

Growth rate (positive values of 𝜔^∗) against wave number 𝑘^∗ for three values of parameter 𝜐^∗=0.0,2.0,5.0, keeping the other parameters fixed 𝐿^∗_𝜌=1.0,  𝜆^∗=1.0,  𝐿^∗_𝑇=1.0.