Radio Recombination Lines

Description

This book is a comprehensive guide to the physics and observations of Radio Recombination Lines from astronomical sources, written for astronomers, physicists, and graduate students. It is suitable for a graduate-level textbook. It includes the history of RRL detections, the astrophysics underlying their intensities and line shapes including topics like departures from LTE and Stark broadening, the maximum possible size of an atom, as well as detailed descriptions of the astronomical topics for which RRLs have proved to be effective tools. The text includes more than 250 equations and 110 illustrations. It also contains hundreds of specific references to the astronomical literature to enable readers to explore additional details. The appendix includes supplementary information such as the detailed physics underlying the Bohr atomic model, tables of RRL frequencies including fine structure components, techniques for calculating hydrogenic oscillator strengths, FORTRAN code for calculating departure coefficients, and a discussion with formulas for converting observational (telescope) intensity units to astrophysical ones.

Subjects

Series Statement

• Astrophysics and Space Science Library, 0067-0057 -- 282

Links

• SpringerLink

Other Editions

• Radio Recombination Lines: Their Physics and Astronomical Applications[electronic resource] :Springer Netherlands2002-01-01
• Radio Recombination LinesIsland Press1990-01-01
• Radio Recombination LinesSpringer London, Limited2009-01-01
• Radio Recombination LinesSpringer2012-01-01