Description
Book SynopsisAn Introduction to Molecular Clouds describes the formation of molecular clouds and the innovative features of molecular clouds with different physical parameters. In this book, Jean-gravitational instability is discussed with different physical parameters, which is the major cause of the formation of molecular clouds in the interstellar medium (ISM), and the way molecular clouds are formed in the astrophysical plasma environment is described. The authors aim to determine the basic conditions responsible for the formation of heavenly bodies in the universe. The book deals with radiative instability in a variety of conditions incorporating different physical parameters such as viscosity, rotation, permeability, porosity, thermal conductivity, Hall current, Finite ion Larmor radius corrections, finite electrical resistivity, radiative heat-loss functions and finite electron inertia, both in gaseous plasma and quantum plasma environments.
Table of ContentsPreface; Rotation of Dark Globules; A New Simplistic Equation of a Macroscopic Equilibrium State for Degenerate Neutron Stars; A New P(R)-Relationship for Stellar Structures; Jeans Instability of Rotating Plasma with Radiative Heat-Loss Function and FLR Corrections Flowing Through Porous Medium for Molecular Cloud Configuration; Molecular Cloud Formation via Thermal Instability of Viscous Partially-Ionized Plasma with Neutral Collision and Radiative Heat-Loss Function in Interstellar Medium; Influence of Electron Plasma Frequency on the Evolution of Gravitational Molecular Clouds; Index.
