DETECTION OF NITRIC-OXIDE IN THE DARK CLOUD L134N
Journal or Book Title
The first detection of interstellar nitric oxide (NO) in a cold dark cloud, L134N is reported. Nitric oxide was observed by means of its two 2 Pi 1/2, J = 3/2 - 1/2, rotational transitions at 150.2 and 150.5 GHz, which occur because of Lambda-doubling. The inferred column density for L134N is about 5 x 10 to the 14th/sq cm toward the SO peak in that cloud. This value corresponds to a fractional abundance relative to molecular hydrogen of about 6 x 10 to the -8th and is in good agreement with predictions of quiescent cloud ion-molecule chemistry. NO was not detected toward the dark cloud TMC-1 at an upper limit of 3 x 10 to the -8th or less.
MCGONAGLE, D; ZIURYS, LM; Irvine, William M.; and MINH, YC, "DETECTION OF NITRIC-OXIDE IN THE DARK CLOUD L134N" (1990). ASTROPHYSICAL JOURNAL. 247.
Retrieved from https://scholarworks.umass.edu/astro_faculty_pubs/247
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