Infrared images of reflection nebulae and Orion's Bar: fluorescent molecular hydrogen and the 3.3 μm feature.

Details Infrared images of reflection nebulae and Orion's Bar: fluorescent molecular hydrogen and the 3.3 μm feature. Infrared images of reflection nebulae and Orion's Bar: fluorescent molecular hydrogen and the 3.3 μm feature.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p..87b&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 87 - 92

Physics

2

Reflection Nebulae: Molecular Hydrogen

Scientific paper

Images have been obtained of the (fluorescent) molecular hydrogen 1 - 0 S(1) line, and of the 3.3 μm emission feature, in Orion's Bar and three reflection nebulae. The emission from these species appears to come from the same spatial locations in all sources observed. This suggests that the 3.3 μm feature is excited by the same energetic UV-photons which cause the molecular hydrogen to fluoresce.

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