A Dirty Window

Diffuse and Translucent Molecular Gas in the Interstellar Medium

  • Loris Magnani
  • Steven N. Shore

Part of the Astrophysics and Space Science Library book series (ASSL, volume 442)

Table of contents

  1. Front Matter
    Pages i-xix
  2. Loris Magnani, Steven N. Shore
    Pages 1-27
  3. Loris Magnani, Steven N. Shore
    Pages 29-67
  4. Loris Magnani, Steven N. Shore
    Pages 69-106
  5. Loris Magnani, Steven N. Shore
    Pages 107-129
  6. Loris Magnani, Steven N. Shore
    Pages 131-153
  7. Loris Magnani, Steven N. Shore
    Pages 155-183
  8. Loris Magnani, Steven N. Shore
    Pages 185-204
  9. Loris Magnani, Steven N. Shore
    Pages 205-225
  10. Loris Magnani, Steven N. Shore
    Pages 227-248
  11. Loris Magnani, Steven N. Shore
    Pages 249-266
  12. Loris Magnani, Steven N. Shore
    Pages 267-294
  13. Loris Magnani, Steven N. Shore
    Pages 295-296
  14. Back Matter
    Pages 297-306

About this book

Introduction

This book provides an introduction to the physics of interstellar gas in the Galaxy. It deals with the diffuse interstellar medium which supplies a complex environment for exploring the neutral gas content of a galaxy like the Milky Way and the techniques necessary for studying this non-stellar component. After an initial exposition of the phases of the interstellar medium and the role of gas in a spiral galaxy, the authors discuss the transition from atomic to molecular gas. They then consider basic radiative transfer and molecular spectroscopy with particular emphasis on the molecules useful for studying low-density molecular gas. Observational techniques for investigating the gas and the dust component of the diffuse interstellar medium throughout the electromagnetic spectrum are explored emphasizing results from the recent Herschel and Planck missions. A brief exposition on dust in the diffuse interstellar medium is followed by a discussion of molecular clouds in general and high-latitude molecular clouds in particular. Ways of calibrating CO observations with the molecular hydrogen content of a cloud are examined along with the dark molecular gas controversy. High-latitude molecular clouds are considered in detail as vehicles for applying the techniques developed in the book. Given the transient nature of diffuse and translucent molecular clouds, the role of turbulence in the origin and dynamics of these objects is examined in some detail.

The book is targeted at graduate students or postdocs who are entering the field of interstellar medium studies.

Keywords

Diffuse Interstellar Medium Book Galactic Molecular Clouds Interstellar Dust Molecular Interstellar Medium Observation of the Diffuse Interstellar Medium Radiative Transfer in the Diffuse Interstellar Medium Theory of the Diffuse Interstellar Medium Turbulence the Diffuse Interstellar Medium

Authors and affiliations

  • Loris Magnani
    • 1
  • Steven N. Shore
    • 2
  1. 1.Department of Physics and AstronomyThe University of GeorgiaAthensUSA
  2. 2.Dipartimento di Fisica “E. Fermi”Università di PisaPisaItaly

Bibliographic information

  • DOI https://doi.org/10.1007/978-3-662-54350-4
  • Copyright Information Springer-Verlag GmbH Germany 2017
  • Publisher Name Springer, Berlin, Heidelberg
  • eBook Packages Physics and Astronomy
  • Print ISBN 978-3-662-54348-1
  • Online ISBN 978-3-662-54350-4
  • Series Print ISSN 0067-0057
  • Series Online ISSN 2214-7985
  • About this book