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Detection of interstellar vibrationally excited HCN

Journal Article · · Astrophys. J., Lett. Ed.; (United States)
DOI:https://doi.org/10.1086/184595· OSTI ID:6099680
Vibrationally excited HCN has been observed for the first time in the interstellar medium. The J = 3-2 rotational transitions of the l-doubled (0,1/sup 1d/,1c, 0) bending mode of HCN have been detected toward Orion-KL and IRC +10216. In Orion, the overall column density in the (0,1,0) mode, which exclusively samples the ''hot core,'' is 1.7-10/sup 16/ cm/sup -2/ and can be understood in terms of the ''doughnut'' model for Orion. The ground-state HCN column density implied by the excited-state observations is 2.3 x 10/sup 18/ cm/sup -2/ in the hot core, at least one order of magnitude greater than the column densities derived for HCN in its spike and plateau/doughnut components. Radiative excitation by 14 ..mu..m flux from IRc2 accounts for the (0,1,0) population provided the hot core is approx.6-7 x 10/sup 16/ cm distant from IRc2, in agreement with the ''cavity'' model for KL. Toward IRC +10216 we have detected J = 3-2 transitions of both (0,1/sup 1c/,/sup 1d/,0) and (0,2/sup 0/,0) excited states. The spectral profiles have been modeled to yield abundances and excitation conditions throughout the expanding envelope.
Research Organization:
Five College Radio Astronomy Observatory, University of Massachusetts, Amherst
OSTI ID:
6099680
Journal Information:
Astrophys. J., Lett. Ed.; (United States), Journal Name: Astrophys. J., Lett. Ed.; (United States) Vol. 300:1; ISSN AJLEA
Country of Publication:
United States
Language:
English