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2000ApJ...538..275J - Astrophys. J., 538, 275-288 (2000/July-3)
The properties of molecular hydrogen toward the Orion belt stars from observations by the interstellar medium absorption profile spectrograph.
JENKINS E.B., WOZNIAK P.R., SOFIA U.J., SONNEBORN G. and TRIPP T.M.
Abstract (from CDS):
For both stars, the H2 absorption features are separated into two velocity components. Total H2 column densities toward δ and ε Ori are 5.5x1014 and 1.9x1016 cm–2, respectively. When these values are compared to the column densities of H I, the fractions of H atoms bound in molecular form 2N(H2)/[2N(H2)+N(H I)]=7x10–6 for δ and 1.3x10–4 for ε. The rotation temperatures of the molecules with J>2 toward ε Ori indicate that the gas is in the general vicinity of the stars that emit UV fluxes capable of rotationally pumping the molecules. For the strongest component of H2 toward δ Ori, the pumping rate is lower and consistent with a general UV flux level in the plane of the Galaxy.
Abstract Copyright: ∼
Journal keyword(s): ISM: Molecules - stars: individual (δ Orionis A, ε Orionis, ζ Orionis A) - Ultraviolet: ISM
Simbad objects: 17
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