Phillips, J. P. and White, Glenn J.
|Google Scholar:||Look up in Google Scholar|
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 Item|
|Copyright Holders:||1982 Not known|
|Extra Information:||ESA The Scientific Importance of Submillimeter Observations
(SEE N83-22034 11-88)
|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/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||07 Jun 2012 07:56|
|Last Modified:||04 Oct 2016 11:18|
|Share this page:|