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Velocity profiles of high-excitation molecular hydrogen linesProfiles of three lines of molecular hydrogen near 2.2 microns, originating from widely spaced energy levels, have been measured at a resolution of 32 km/s at Peak 1 in the Orion molecular outflow. The three lines, 1 - 0 S(1), 2 - 1 S(1), and 3 - 2 S(3), are found to have identical profiles. This result rules out any significant contribution to the population of the higher energy levels of molecular hydrogen at Peak 1 by fluorescence, and is generally consistent with emission from multiple J-type shocks.
Document ID
19900033179
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Moorhouse, A.
(Edinburgh Univ. United Kingdom)
Brand, P. W. J. L.
(Edinburgh, University United Kingdom)
Geballe, T. R.
(Joint Astronomy Center Hilo, HI, United States)
Burton, M. G.
(NASA Ames Research Center Moffett Field; California, University, Irvine, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Publication Information
Publication: Royal Astronomical Society, Monthly Notices
Volume: 242
ISSN: 0035-8711
Subject Category
Astrophysics
Accession Number
90A20234
Distribution Limits
Public
Copyright
Other

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