As demonstrated by five Nobel Prizes in physics, radio astronomy has contributed greatly to our understanding of the Universe. Yet for too long, there has been no comprehensive textbook on radio astronomy for undergraduate students.
This two-volume set of introductory textbooks is exclusively devoted to radio astronomy, with extensive discussions of telescopes, observation methods, and astrophysical processes that are relevant for this exciting field.
The first volume, Fundamentals of Radio Astronomy: Observational Methods, discusses radio astronomy instrumentation and the techniques to conduct successful observations. The second volume, Fundamentals of Radio Astronomy: Astrophysics, discusses the physical processes that give rise to radio emission, presents examples of astronomical objects that emit by these mechanisms, and illustrates how the relevant physical parameters of astronomical sources can be obtained from the radio observations.
Requiring no prior knowledge of astronomy, the two volumes are ideal textbooks for radio astronomy courses at the undergraduate or graduate level, particularly those that emphasize radio wavelength instrumentation and observational techniques or the astrophysics of radio sources. The set enables instructors to pick and choose topics from the two volumes that best fit their courses.
- Explores radio astronomy instruments and techniques that are important to enable observations
- Describes astrophysical processes that produce the radio emissions observed in different types of astronomical objects
- Includes numerous worked examples to demonstrate how the methods are used to solve problems, in addition to advanced material for students with more extensive physics and mathematics backgrounds
Table of Contents
Observational Methods and Astrophysics - Two Volume Set
Volumen One: Observational Methods Chapter 1. Introductory Material. Chapter 2. Introduction to Radiation Physics. Chapter 3. Radio Telescopes. Chapter 4. Single-Dish Radio Telescope Observations. Chapter 5. Aperture Synthesis Basics: Two-Element Interferometers. Chapter 6. Aperture Synthesis: Advanced Discussion. Appendices
Volume Two: Astrophysics. Chapter 1. Introduction. Chapter 2. Propagation of Radiation. Chapter 3. Continuum Emission Processes. Chapter 4. Spectral Lines. Chapter 5. The Cold Interstellar Medium of the Milky Way. Chapter 6. HII Regions and Planetary Nebulae at Radio Wavelengths. Chapter 7. Radio Emission from Stellar Objects. Chapter 8. Galaxies at Radio Wavelengths. Chapter 9. Radio Galaxies and Quasars. Chapter 10. Cosmic Microwave Background. Appendices
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.
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.