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1994ApJ...423..326B - Astrophys. J., 423, 326-333 (1994/March-1)
Spectral imaging of the Orion bar at 3.3, 8.4 and 11.3 microns : comparison with a fluorescent polycyclic aromatic hydrocarbon model.
BREGMAN J., LARSON K., RANK D. and TEMI P.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): ISM: Dust, Extinction - Infrared: ISM: Continuum - ISM: Individual Name: Orion Nebula - ISM: Molecules
Simbad objects: 2
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