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Radio Recombination Lines
Peter A. . Ed(S): Shaver
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Description for Radio Recombination Lines
Paperback. Proceedings of a Workshop held in Ottawa, Canada, August 24-25, 1979 Editor(s): Shaver, Peter A. Series: Astrophysics and Space Science Library. Num Pages: 299 pages, biography. BIC Classification: PG; WNX. Category: (P) Professional & Vocational. Dimension: 234 x 156 x 16. Weight in Grams: 468.
Since their first detection 15 years ago, radio recombination lines from several elements have been observed in a wide variety of objects including HII regions, planetary nebulae, molecular clouds, the diffuse interstellar medium, and recently, other galaxies. The observations span almost the entire range from 0.1 to 100 GHz, and employ both single djsh and aperture synthesis techniques. The theory of radio recombination lines has also advanced strongly, to the point where it is perhaps one of the best-understood in astro physics. In a parallel development, it has become possible over the last decade to study these same highly-excited atoms ... Read more
Since their first detection 15 years ago, radio recombination lines from several elements have been observed in a wide variety of objects including HII regions, planetary nebulae, molecular clouds, the diffuse interstellar medium, and recently, other galaxies. The observations span almost the entire range from 0.1 to 100 GHz, and employ both single djsh and aperture synthesis techniques. The theory of radio recombination lines has also advanced strongly, to the point where it is perhaps one of the best-understood in astro physics. In a parallel development, it has become possible over the last decade to study these same highly-excited atoms ... Read more
Product Details
Format
Paperback
Publication date
2011
Publisher
Springer Netherlands
Number of pages
299
Condition
New
Series
Astrophysics and Space Science Library
Number of Pages
289
Place of Publication
Dordrecht, Netherlands
ISBN
9789400990265
SKU
V9789400990265
Shipping Time
Usually ships in 15 to 20 working days
Ref
99-15
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