Excitation conditions in the Orion molecular cloud obtained from observations of ortho- and para-lines of H$_ {\sf 2}$
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20065786/pdf
Reference85 articles.
1. Explosive ejection of matter associated with star formation in the Orion nebula
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5. Submillimeter Array 440 μm/690 GHz Line and Continuum Observations of Orion KL
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