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Interstellar silicon sulfide
- Source :
- Astrophysical Journal.
- Publication Year :
- 1981
- Publisher :
- United States: NASA Center for Aerospace Information (CASI), 1981.
-
Abstract
- Silicon sulfide has been observed in Sgr B2 at 108.92 GHz and 90.77 GHz and in Orion A at 108.92 GHz. The column density is 1-2 x 10 to the 13th/sq cm in both sources. SiS was not seen in two other molecular clouds where SiO has been detected; nor was it seen in a variety of late-type stars with varying C/O ratios. It appears that SiS is significantly less abundant than SiO in the interstellar medium and probably at least somewhat less abundant in oxygen-rich late-type variable stars.
- Subjects :
- Astrophysics
Subjects
Details
- Language :
- English
- Database :
- NASA Technical Reports
- Journal :
- Astrophysical Journal
- Notes :
- NAS7-100
- Publication Type :
- Report
- Accession number :
- edsnas.19810059435
- Document Type :
- Report
- Full Text :
- https://doi.org/10.1086/159015