| 書目名稱 | Radio Recombination Lines |
| 副標(biāo)題 | Their Physics and As |
| 編輯 | M. A. Gordon,R. L. Sorochenko |
| 視頻video | http://file.papertrans.cn/821/820641/820641.mp4 |
| 概述 | Includes supplementary material: |
| 叢書名稱 | Astrophysics and Space Science Library |
| 圖書封面 |  |
| 描述 | 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 |
| 出版日期 | Book 2002 |
| 關(guān)鍵詞 | astronomy; astrophysics; spectra; stars; stellar |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-94-010-0261-5 |
| isbn_softcover | 978-94-010-3956-7 |
| isbn_ebook | 978-94-010-0261-5Series ISSN 0067-0057 Series E-ISSN 2214-7985 |
| issn_series | 0067-0057 |
| copyright | Kluwer Academic Publishers 2002 |
|Archiver|手機(jī)版|小黑屋|
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