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

Figure 6

Growth rate (positive values of 𝜔^∗) against wave number 𝑘^∗  for several values of parameter 𝜐^∗₀  keeping the other parameters fixed 𝐿^∗_𝜌=0.5,  𝐿^∗_𝑇=0.5,  𝜆^∗=1.0,  𝑉^∗=1.0,  𝜂^∗=0.5.  𝜐^∗=0.0: (1)  𝜐^∗₀=0.0, (2) 𝜐^∗₀=1.5 (3) 𝜐^∗₀=3.0.  𝜐^∗=0.9: (4) 𝜐^∗₀=1.5, (5) 𝜐^∗₀=3.0.