| 書(shū)目名稱 | CO: Twenty-Five Years of Millimeter-Wave Spectroscopy | | 副標(biāo)題 | Proceedings of the 1 | | 編輯 | William B. Latter,Simon J. E. Radford,John Bally | | 視頻video | http://file.papertrans.cn/221/220410/220410.mp4 | | 叢書(shū)名稱 | International Astronomical Union Symposia | | 圖書(shū)封面 |  | | 描述 | Interstellar carbon monoxide (CO) was first detected in 1970 with the 36 foot diameter telescope of the National Radio Astronomy Observatory! on Kitt Peak in Southern Arizona. R. W. Wilson, K. B. Jefferts, and A. A. Penzias of Bell Labs reported, "We have found intense 2.6 mm line radiation 2 from nine Galactic sources which we attribute to carbon monoxide." Soon afterward, several other basic molecules were also observed in space. IAU Symposium 170, CO: Twenty Five Years of Millimeter Wave Spectroscopy, was organized to commemorate those discoveries. The Symposium reviewed the accomplishments of a quarter century of research on interstellar molec- ular gas, surveyed the current state of millimeter-wave spectroscopy, and gave a glimpse of what the next 25 years might hold. Studies of interstellar CO have revolutionized our understanding of the phases and dynamics of the interstellar medium, the initial and final stages of stellar evolution, the chemistry of dense and diffuse interstellar matter and of the solar system, the structure of the Milky Way galaxy, and the content and structure of other galaxies, some very distant. Spectroscopic studies of CO and other molecules are primar | | 出版日期 | Conference proceedings 1997 | | 關(guān)鍵詞 | astronomy; astrophysics; galaxy; interstellar matter; milky way; observatory; planet; radio astronomy; solar | | 版次 | 1 | | doi | https://doi.org/10.1007/978-94-011-5414-7 | | isbn_softcover | 978-0-7923-4284-7 | | isbn_ebook | 978-94-011-5414-7Series ISSN 1743-9213 Series E-ISSN 2352-2186 | | issn_series | 1743-9213 | | copyright | Springer Science+Business Media Dordrecht 1997 |
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