Fundamentals of Radio Astronomy

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A01=Jonathan Marr
A01=Ronald L. Snell
A01=Stanley Kurtz
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AGN
Author_Jonathan Marr
Author_Ronald L. Snell
Author_Stanley Kurtz
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Brightness Temperature
Category1=Non-Fiction
Category=PHJ
Category=PHVB
Category=THR
CMB
CMB Photon
CMB Power Spectrum
Column Density
COP=United States
Cosmic Microwave Background
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Early Type Galaxies
Energy Density
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eq_science
Excitation Temperature
Flux Density
Free Free Emission
Galactic Center
Galactic Longitude
HII Region
Language_English
LCP Wave
Molecular Cloud
Molecular Gas
Optical Depth
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Price_€100 and above
PS=Active
Radio Galaxies
Rotation Curve
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Solar Radio Emission
Star Formation Rate
Stellar Mass
Synchrotron Radiation

Product details

  • ISBN 9781498725774
  • Weight: 982g
  • Dimensions: 178 x 254mm
  • Publication Date: 14 May 2019
  • Publisher: Taylor & Francis Inc
  • Publication City/Country: US
  • Product Form: Hardback
  • Language: English
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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

Ronald L. Snell is a professor of astronomy at the University of Massachusetts, Amherst. His research interests include the physical and chemical properties of molecular clouds, star formation, and molecular outflows; he also has extensive experience observing at radio wavelengths. He earned a PhD in astronomy from the University of Texas at Austin.

Stanley E. Kurtz is a professor of radio astronomy and astrophysics at the National Autonomous University of Mexico. His research interests include massive star formation, the interstellar medium, and radio astronomy instrumentation and techniques. He earned a PhD in physics from the University of Wisconsin at Madison.

Jonathan M. Marr is a senior lecturer of physics and astronomy at Union College. His research involves high-resolution, radio-wavelength observations of radio galaxies and the Galactic center. He earned a PhD in astronomy from the University of California, Berkeley.