Paper
21 April 1986 Submillimetre Wave Spectroscopy In Astronomy Related To The ESA-project FIRST (Far Infrared Submillimetre Space Telescope)
G. Winnewisser
Author Affiliations +
Proceedings Volume 0598, Instrumentation for Submillimeter Spectroscopy; (1986) https://doi.org/10.1117/12.952311
Event: 1985 International Technical Symposium/Europe, 1985, Cannes, France
Abstract
The scientific objectives of a submillimetre heterodyne mission are summarized. Interstellar submillimetre wave radiation emanates from a wide diversity of "cool" astronomical objects ranging from the recombination era of the early universe to circumstellar shells of late type stars and planetary atmospheres within the solar system. The present design status of the Far-Infrared and Submillimetre Space Telescope (FIRST) is reported. Some recent new scientific observations pertaining to interstellar molecular submillimetre spectroscopy are reviewed.
© (1986) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
G. Winnewisser "Submillimetre Wave Spectroscopy In Astronomy Related To The ESA-project FIRST (Far Infrared Submillimetre Space Telescope)", Proc. SPIE 0598, Instrumentation for Submillimeter Spectroscopy, (21 April 1986); https://doi.org/10.1117/12.952311
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Cited by 3 scholarly publications.
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KEYWORDS
Molecules

Clouds

Astronomy

Stars

Galactic astronomy

Molecular spectroscopy

Heterodyning

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