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Interstellar Processes

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Cover of 'Interstellar Processes'

Table of Contents

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    Book Overview
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    Chapter 1 The Milky Way as a Galaxy
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    Chapter 2 H2 in the Galaxy
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    Chapter 3 Molecular Clouds: An Overview
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    Chapter 4 Observations of Molecular Cloud Structure and Internal Motions
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    Chapter 5 The Atomic Component
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    Chapter 6 Hot Interstellar Gas in the Galactic Disk and Halo
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    Chapter 7 The High-Energy Component of the ISM—Cosmic-Ray Phenomena
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    Chapter 8 Interstellar Magnetic Fields
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    Chapter 9 The Theory of the Galactic Magnetic Field
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    Chapter 10 Panel Discussion: Phases of the Interstellar Medium
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    Chapter 11 Mass and Energy Balance in the Interstellar Medium: How to Model the Disk Gas in our Galaxy
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    Chapter 12 Cloud Formation and Destruction
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    Chapter 13 The Physics of Interstellar Shock Waves
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    Chapter 14 Theory of Collapse and Protostar Formation
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    Chapter 15 Theoretical Approaches to Interstellar Turbulence
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    Chapter 16 Composition, Structure, and Chemistry of Interstellar Dust
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    Chapter 17 Infrared Absorption and Emission Characteristics of Interstellar PAHs
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    Chapter 18 Grain Destruction, Formation, and Evolution
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    Chapter 19 Interstellar Grains in the Solar System
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    Chapter 20 Element Abundances in the Interstellar Atomic Material
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    Chapter 21 Chemical Abundances in Molecular Clouds
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    Chapter 22 Gas Phase Chemical Processes in Molecular Clouds
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    Chapter 23 Chemical Evolution of Molecular Clouds
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    Chapter 24 Chemical Evolution of Galaxies
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    Chapter 25 The Solar System/Interstellar Medium Connection: Gas Phase Abundances
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    Chapter 26 Observations of the Cooling of the Interstellar Gas
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    Chapter 27 Heating and Cooling of the Interstellar Gas
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    Chapter 28 Atomic and Molecular Physics of Interstellar Heating and Cooling
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    Chapter 29 Masers in the Interstellar Medium
Overall attention for this book and its chapters
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About this Attention Score

  • In the top 25% of all research outputs scored by Altmetric
  • High Attention Score compared to outputs of the same age (97th percentile)
  • High Attention Score compared to outputs of the same age and source (96th percentile)

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