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Titlebook: CO: Twenty-Five Years of Millimeter-Wave Spectroscopy; Proceedings of the 1 William B. Latter,Simon J. E. Radford,John Bally Conference pro

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書目名稱CO: Twenty-Five Years of Millimeter-Wave Spectroscopy
副標題Proceedings of the 1
編輯William B. Latter,Simon J. E. Radford,John Bally
視頻videohttp://file.papertrans.cn/221/220410/220410.mp4
叢書名稱International Astronomical Union Symposia
圖書封面Titlebook: CO: Twenty-Five Years of Millimeter-Wave Spectroscopy; Proceedings of the 1 William B. Latter,Simon J. E. Radford,John Bally Conference pro
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
doihttps://doi.org/10.1007/978-94-011-5414-7
isbn_softcover978-0-7923-4284-7
isbn_ebook978-94-011-5414-7Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightSpringer Science+Business Media Dordrecht 1997
The information of publication is updating

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A Molecular Worm in Scutumrvations have so far been confined mainly to several vertical strips across the plane covering a few degrees in Galactic longitude and 6°‐8° in Galactic latitude; details of this on-going survey are given in Dame & Thaddeus (1995).
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On the Fractal Structure of Molecular Cloudsmportant to study the power spectrum of observed cloud images. For HI clouds (Green 1993), the azimuthally averaged power spectra derived directly from interferometer observations are well characterized by a power law with a spectral index close to 2.8.
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https://doi.org/10.1007/978-3-319-59957-1sed to determine the CR density and calibrate the CO line as a tracer of molecular mass. Dominant production mechanisms for γ rays of energies ~30 MeV-30 GeV are the decay of pions produced in collisions of CR protons with ambient matter and Bremsstrahlung scattering of CR electrons.
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