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1986ApJ...302..693G - Astrophys. J., 302, 693-700 (1986/March-0)
Comparison of 2.1 and 3.8 micron line profiles of shocked H2 in the Orion molecular cloud.
GEBALLE T.R., PERSSON S.E., SIMON T., LONSDALE C.J. and McGREGOR P.J.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Infrared: Spectra - Interstellar: Molecules - Line Formation - Line Profiles - Nebulae: Orion Nebula - Shock Waves
Simbad objects: 2
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