Radio Recombination Lines - Their Physics and Astronomical Applications (Paperback, Softcover reprint of the original 1st ed. 2002)

Recombination lines at radio wavelengths have been - and still are - a pow erful tool for modern astronomy. For more than thirty years they have allowed astronomers to probe the gases from which stars form. They have even been detected in the Sun. In addition, observations of these spectral lines facilitate basic research into the atom, in forms and environments that can only exist in the huge dimensions and extreme conditions of cosmic laboratories. We intend this book to serve as a tourist's guide to the world of Radio Recombination Lines. It contains three divisions: a history of their discovery, the physics of how they form and how their voyage to us influences their spectral profiles, and a description of their many astronomical contributions to date. The appendix includes supplementary calculations that may be useful to some astronomers. This material also includes tables of line frequencies from 12 MHz to 30THz (AlOJLm) as well as FORTRAN computer code to calculate the fine structure components of the lines, to evaluate radial matrix integrals, and to calculate the departure coefficients of hydrogen in a cosmic environment. It also describes how to convert observational to astrophysical units. The text includes extensive references to the literature to assist readers who want more details.

General

Imprint:	Springer
Country of origin:	Netherlands
Series:	Astrophysics and Space Science Library, 282
Release date:	September 2012
First published:	2002
Authors:	M.A. Gordon • Roman L. Sorochenko
Dimensions:	240 x 160 x 20mm (L x W x T)
Format:	Paperback
Pages:	358
Edition:	Softcover reprint of the original 1st ed. 2002
ISBN-13:	978-9401039567
Categories:	Books > Science & Mathematics > Astronomy, space & time > General Books > Science & Mathematics > Physics > Nuclear structure physics Promotions
LSN:	9401039569
Barcode:	9789401039567

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