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Interstellar silicon sulfide

Authors :
Dickinson, D. F
Kuiper, E. N. R
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

Subjects :
Astrophysics

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