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Fundamentals of Radio Astronomy : Astrophysics

By: (Author) Jonathan Marr , (Author) Ronald L. Snell , (Author) Stanley Kurtz

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Ksh 20,700.00

Format: Hardback or Cased Book

ISBN-10: 1498725775

ISBN-13: 9781498725774

Series: Series in Astronomy and Astrophysics

Publisher: Taylor & Francis Inc

Imprint: CRC Press Inc

Country of Manufacture: US

Country of Publication: GB

Publication Date: May 14th, 2019

Print length: 360 Pages

Weight: 918 grams

Dimensions (height x width x thickness): 18.20 x 26.00 x 2.40 cms

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This undergraduate textbook presents an extensive introduction to the astrophysical processes that enable radio astronomy. It discusses the physical phenomena that give rise to radio emissions, presenting examples of astronomical objects, and illustrating how the physical parameters of astronomical sources can be obtained from radio observations.

As demonstrated by five Nobel Prizes in physics, radio astronomy has contributed greatly to our understanding of the Universe. Courses covering this subject are, therefore, very important in the education of the next generation of scientists who will continue to explore the Cosmos.

This textbook, the second of two volumes, presents an extensive introduction to the astrophysical processes that are studied in radio astronomy. Suitable for undergraduate courses on radio astronomy, it discusses the physical phenomena that give rise to radio emissions, presenting examples of astronomical objects, and illustrating how the relevant physical parameters of astronomical sources can be obtained from radio observations.

Unlike other radio astronomy textbooks, this book provides students with an understanding of the background and the underlying principles, with derivations available for most of the equations used in the textbook.

Features:

  • Presents a clear and concise discussion of the important astronomical concepts and physical processes that give rise to both radio continuum and radio spectral line emission
  • Discusses radio emissions from a variety of astronomical sources and shows how the observed emissions can be used to derive the physical properties of these sources
  • Includes numerous examples using actual data from the literature


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