An Introduction to Molecular Clouds

$82.00

Series: Advances in Astronomy and Astrophysics

BISAC: SCI005000

An 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.

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Table of Contents

Preface

Chapter 1. Rotation of Dark Globules
(A. L. Gyulbudaghian – Victor Ambartsumian Byurakan Observatory)

Chapter 2. A New Simplistic Equation of a Macroscopic Equilibrium State for Degenerate Neutron Stars.
(Rohaan Deb – Department of Physics, Rheinische Friedrich-Wilhelms-Universität Bonn, Bonn, Germany and Pralay Kumar Karmakar – Department of Physics, Tezpur University, Napaam, Tezpur, Assam, India)

Chapter 3. A New P(R)-Relationship for Stellar Structures
(Rohaan Deb – Department of Physics, Rheinische Friedrich-Wilhelms-Universität Bonn, Bonn, Germany and Pralay Kumar Karmakar – Department of Physics, Tezpur University, Napaam, Tezpur, Assam, India)

Chapter 4. Jeans Instability of Rotating Plasma with Radiative Heat-Loss Function and FLR Corrections Flowing Through Porous Medium for Molecular Cloud Configuration
(Sachin Kaothekar – Department of Physics, Mahakal Institute of Technology & Management, Ujjain (M.P.), India)

Chapter 5. Molecular Cloud Formation via Thermal Instability of Viscous Partially-Ionized Plasma with Neutral Collision and Radiative Heat-Loss Function in Interstellar Medium
(G.D. Soni and Sachin Kaothekar – Government Science College, Dewas, Madhya Pradesh, India, et al.)

Chapter 6. Influence of Electron Plasma Frequency on the Evolution of Gravitational Molecular Clouds
(D. L. Sutar, R. K. Pensia, A. K. Patidar, and V. Shrivastva – Department of Physics, Government RV College Manasa (MP), India, et al.)

Index

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