Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237.1009b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, April 15, 1989, p. 1009-1018.
Astronomy and Astrophysics
Astronomy
38
Hydrogen Clouds, Line Spectra, Orion Nebula, Bow Waves, Molecular Clouds, Shock Waves, Star Formation, Supersonic Flow, Velocity Distribution
Scientific paper
The profile of the 1-OS(1) line of molecular hydrogen at Peak 1 is
presented, and is shown to pose problems for many models of the
excitation region.
Brand Peter W. J. L.
Geballe Thomas Ronald
Toner M. P.
Webster Adrian S.
No associations
LandOfFree
The velocity profile of the 1-O S(1) line of molecular hydrogen at Peak 1 in Orion does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The velocity profile of the 1-O S(1) line of molecular hydrogen at Peak 1 in Orion, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The velocity profile of the 1-O S(1) line of molecular hydrogen at Peak 1 in Orion will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1738712