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X-Ray Emission from Clusters of Galaxies

X-Ray Emission from Clusters of Galaxies

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"X-Ray Emission from Clusters of Galaxies" by Craig L. Sarazin is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

First published in 1988, this book is a comprehensive survey of the astrophysical characteristics of the hot gas which pervades clusters of galaxies. In our universe, clusters of galaxies are the largest organised structures. Typically they comprise hundreds of galaxies moving through a region of space ten million light years in diameter. The volume between the galaxies is filled with gas having a temperature of 100 million degrees. This material is a strong source of cosmic X-rays. Dr Sarazin describes the theoretical description of the origin, dynamics, and physical state of the cluster gas. Observations by radio and optical telescopes are also summarised. This account is addressed to professional astronomers and to graduate students. It is an exhaustive summary of a rapidly expanding field of research in modern astrophysics.

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Best For: Researchers and students in astrophysics focusing on galaxy clusters and high-energy phenomena.
Focus: Astrophysical properties and X-ray emissions of hot gas in galaxy clusters.
Covers: Physical characteristics of hot intracluster gas, temperature measurements, and spatial distribution within clusters.
Why It Matters: Understanding the hot gas in galaxy clusters helps reveal the structure and dynamics of the largest organized systems in the universe.

"X-Ray Emission from Clusters of Galaxies" by Craig L. Sarazin is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

Topic: Deep Sky & Solar System

Author: Craig L. Sarazin

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

First published in 1988, this book is a comprehensive survey of the astrophysical characteristics of the hot gas which pervades clusters of galaxies. In our universe, clusters of galaxies are the largest organised structures. Typically they comprise hundreds of galaxies moving through a region of space ten million light years in diameter. The volume between the galaxies is filled with gas having a temperature of 100 million degrees. This material is a strong source of cosmic X-rays. Dr Sarazin describes the theoretical description of the origin, dynamics, and physical state of the cluster gas. Observations by radio and optical telescopes are also summarised. This account is addressed to professional astronomers and to graduate students. It is an exhaustive summary of a rapidly expanding field of research in modern astrophysics.

AuthorCraig L. Sarazin
PublisherCambridge University Press
Published2009-06-18
ISBN-139780521113137
BindingPaperback
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System
SeriesCambridge Astrophysics

Format: Paperback

Language: English

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