Rate constants for the formation of CS by radiative association
Abstract
Rate constants for the formation of carbon monosulfide (CS) by radiative association are calculated using accurate molecular data. The rate constants include both direct and indirect formation processes. The indirect processes (inverse rotational and electronic predissociation) are evaluated for conditions of local thermodynamic equilibrium (LTE) and also in the non-LTE limit of zero radiation temperature and atomic density. Phenomenological rate constants for CS formation in realistic astrophysical environments are expected to lie in-between these limiting cases. An analytic formula is used to fit the rate constants for convenient use in astrophysical models. The impact of the results on various astrophysical environments is briefly discussed.
- Authors:
-
- Pennsylvania State Univ., Reading, PA (United States)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Univ. of Georgia, Athens, GA (United States)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Queen's Univ., Belfast, Northern Ireland (United Kingdom)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1543963
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 479; Journal Issue: 4; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics
Citation Formats
Forrey, R. C., Babb, J. F., Stancil, P. C., and McLaughlin, B. M. Rate constants for the formation of CS by radiative association. United States: N. p., 2018.
Web. doi:10.1093/mnras/sty1739.
Forrey, R. C., Babb, J. F., Stancil, P. C., & McLaughlin, B. M. Rate constants for the formation of CS by radiative association. United States. https://doi.org/10.1093/mnras/sty1739
Forrey, R. C., Babb, J. F., Stancil, P. C., and McLaughlin, B. M. Sat .
"Rate constants for the formation of CS by radiative association". United States. https://doi.org/10.1093/mnras/sty1739. https://www.osti.gov/servlets/purl/1543963.
@article{osti_1543963,
title = {Rate constants for the formation of CS by radiative association},
author = {Forrey, R. C. and Babb, J. F. and Stancil, P. C. and McLaughlin, B. M.},
abstractNote = {Rate constants for the formation of carbon monosulfide (CS) by radiative association are calculated using accurate molecular data. The rate constants include both direct and indirect formation processes. The indirect processes (inverse rotational and electronic predissociation) are evaluated for conditions of local thermodynamic equilibrium (LTE) and also in the non-LTE limit of zero radiation temperature and atomic density. Phenomenological rate constants for CS formation in realistic astrophysical environments are expected to lie in-between these limiting cases. An analytic formula is used to fit the rate constants for convenient use in astrophysical models. The impact of the results on various astrophysical environments is briefly discussed.},
doi = {10.1093/mnras/sty1739},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 4,
volume = 479,
place = {United States},
year = {Sat Jun 30 00:00:00 EDT 2018},
month = {Sat Jun 30 00:00:00 EDT 2018}
}
Web of Science
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