A search for interstellar silicon nitride.
Abstract
A search for the N = 2 - 1 rotational transition of SiN at 87 GHz has established that the ratios of the abundances of this compound to CN, toward the four sources Orion-KL, IRC +10216, Sagittarius B2, and DR 21(OH), are significantly less than the Si-to-C ratio of 0.1. These ratios suggest that either Si is depleted onto grains where CN is present, or that ion-molecule chemistry does not favor the production of SiN. Si-30S has been detected toward IRC +10216, and a comparison with Si-28S and Si-29S yields terrestrial isotopic abundance ratios for Si.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- June 1984
- DOI:
- 10.1086/162091
- Bibcode:
- 1984ApJ...281..219Z
- Keywords:
-
- Astronomical Spectroscopy;
- Interstellar Chemistry;
- Interstellar Matter;
- Silicon Nitrides;
- Abundance;
- Line Spectra;
- Astrophysics