Suitable for final year undergraduates and graduate students studying astronomy or astrophyics, this volume explores the physics of many interesting situations in the interstellar medium, assuming a knowledge possessed by university physics students. In addition, prospective research students and scientists in related fields will find the discussion of the astronomical environment and the effect of the interstellar medium on galactic evolution of interest.
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5 of 6 people found the following review helpful:
4.0 out of 5 stars
Good Introductory Text,
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This review is from: The Physics of the Interstellar Medium, Second Edition (Series in Astronomy and Astrophysics) (Paperback)
A concise and clear introduction to the interstellar medium. Chapters 5 to 7 on radiatively excited regions and gas dynamics are particularly well written (half the book). The rest of the book is perhaps too concise to cover adequately topics such as dust properties and star formation.
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First Sentence:
I f we are fortunate enough to see the sky on a moonless and cloudless night, then, when our eyes have accustomed to the dark, we can discern the prominent feature called the Milky Way. Read the first page Key Phrases - Statistically Improbable Phrases (SIPs): (learn more)
shocked wind gas, stellar wind gas, shocked interstellar gas, energy output rate, specific total energy, sound crossing time, shocked gas, diffuse nebulae, neutral clouds, coronal gas, ionization balance, interstellar gases, ionized region, gas sphere, interstellar medium, grain temperature, shock velocity, interstellar grains, interstellar molecules, radio region, neutral gas, forbidden lines, ionizing photons Key Phrases - Capitalized Phrases (CAPs): (learn more)
David Malin, Milky Way, Copyright Anglo-Australian Observatory, Einstein A-coefficient New!
Books on Related Topics | Concordance | Text Stats Browse Sample Pages:
Front Cover | Table of Contents | First Pages | Index | Back Cover | Surprise Me!
I f we are fortunate enough to see the sky on a moonless and cloudless night, then, when our eyes have accustomed to the dark, we can discern the prominent feature called the Milky Way. Read the first page Key Phrases - Statistically Improbable Phrases (SIPs): (learn more)
shocked wind gas, stellar wind gas, shocked interstellar gas, energy output rate, specific total energy, sound crossing time, shocked gas, diffuse nebulae, neutral clouds, coronal gas, ionization balance, interstellar gases, ionized region, gas sphere, interstellar medium, grain temperature, shock velocity, interstellar grains, interstellar molecules, radio region, neutral gas, forbidden lines, ionizing photons Key Phrases - Capitalized Phrases (CAPs): (learn more)
David Malin, Milky Way, Copyright Anglo-Australian Observatory, Einstein A-coefficient New!
Books on Related Topics | Concordance | Text Stats Browse Sample Pages:
Front Cover | Table of Contents | First Pages | Index | Back Cover | Surprise Me!
Citations (learn more)
This book cites 7
books:
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25
books
cite this book:
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- The Origin and Evolution of the Solar System (Series in Astronomy and Astrophysics) by Michael M. Woolfson in Front Matter
- The Solar System (with AceAstronomy™, Virtual Astronomy Labs Printed Access Card) by Michael A. Seeds in Front Matter
- An Introduction to the Science of Cosmology (Series in Astronomy and Astrophysics) by Derek Raine in Front Matter
- Dust and Chemistry in Astronomy (Series in Astronomy and Astrophysics) by T.J Millar in Front Matter
- Observational Astrophysics, (Graduate Series in Astronomy) by R. E. White in Front Matter
See all 7 books this book cites
- Dust in the Galactic Environment (2nd Edition) (Series in Astronomy and Astrophysics) by D.C.B Whittet in Front Matter, page 36, and Back Matter
- Galaxies in the Universe: An Introduction by Linda S. Sparke on page 109, and Back Matter
- Blowing Bubbles in the Cosmos: Astronomical Winds, Jets, and Explosions by T. W. Hartquist on page 45, and page 66
- Magnetohydrodynamic Turbulence by Dieter Biskamp in Back Matter
- Observational Astrophysics by Robert C. Smith in Back Matter
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