Abstract
A new interstellar molecule, N2O, known as nitrous oxide or 'laughing gas,' has been detected using the NRAO 12 m telescope. The J = 3 - 2, 4 - 3, 5 - 4, and 6 - 5 rotational transitions of this species at 75, 100, 125, and 150 GHz, respectively, were observed toward Sgr B2(M). The column density derived for N2O in this source is N tot approx. 10 15 /sq. cm, which corresponds to a fractional abundance of approx. 10 -9, relative to H2. This value implies abundance ratios of N2O/NO approx. 0.1 and N2O/HNO approx. 3 in the Galactic center. Such ratios are in excellent agreement with predictions of ion-molecule models of interstellar chemistry using early-time calculations and primarily neutral-neutral reactions. N2O is the third interstellar molecule detected thus far containing an N-O bond. Such bonds cannot be so rare as previously thought.
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CITATION STYLE
Ziurys, L. M., Apponi, A. J., Hollis, J. M., & Snyder, L. E. (1994). Detection of interstellar N2O: A new molecule containing an N-O bond. The Astrophysical Journal, 436, L181. https://doi.org/10.1086/187662
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