Abstract
Abstract
Here we present our current update of CLOUDY on gas-phase chemical reactions for the formation and destruction of the SiS molecule, its energy levels, and collisional rate coefficients with H2, H, and He over a wide range of temperatures. As a result, henceforth the spectral synthesis code CLOUDY predicts SiS line intensities and column densities for various astrophysical environments.
Funder
Department of Science and Technology, Ministry of Science and Technology, India
Center for Selective C-H Functionalization, National Science Foundation
NASA
Space Telescope Science Institute
NSF
Publisher
American Astronomical Society
Cited by
1 articles.
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