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The SO 2₃ - 1₂ emission in orion A

Phillips, J. P. and White, Glenn J. (1982). The SO 2₃ - 1₂ emission in orion A. In: Scientific Importance of Submillimetre Observations, 03-04 Dec 1981, Leiden, pp. 33–36.

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Orion A is one of the nearest and best studied regions of star formation, the strongest CO source so far detected, and a particularly fruitful region in the search for new and ever more exotic molecules. A stellar wind, with genesis in some newly formed or forming star, is being power driven into a surrounding placental cloud. The resulting shocks lead to densities of order 1 x 106 1cm-3 or higher, and gas kinetic temperatures T ~ 2000 K, causing excitation of H2 quadrupole emission in the near infrared and the higher rotational transitions of CO in the far-infrared.

Item Type: Conference or Workshop Item
Copyright Holders: 1982 Not known
Extra Information: ESA The Scientific Importance of Submillimeter Observations
(SEE N83-22034 11-88)
pp. 33-36
Keywords: molecular rotation; Orion constellation; quadrupoles; stellar evolution; stellar winds; thermal shock; velocity distribution; carbon monoxide; density (mass/volume); gas temperature; hydrogen; kinematics; molecular clouds; protostars
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 33793
Depositing User: G. J. White
Date Deposited: 07 Jun 2012 07:56
Last Modified: 07 Dec 2018 10:06
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