English

ExoMol line lists XXV: A hot line list for silicon sulphide, SiS

Solar and Stellar Astrophysics 2018-08-21 v1 Earth and Planetary Astrophysics Astrophysics of Galaxies

Abstract

SiS has long been observed in the circumstellar medium of the carbon-rich star IRC+10216 CW Leo. Comprehensive and accurate rotation-vibrational line lists and partition functions are computed for 12 isotopologues of silicon sulphide (28^{28}Si32^{32}S, 28^{28}Si34^{34}S, 29^{29}Si32^{32}S, 28^{28}Si33^{33}S, 30^{30}Si32^{32}S, 29^{29}Si34^{34}S, 30^{30}Si34^{34}S, 28^{28}Si36^{36}S, 29^{29}Si33^{33}S, 29^{29}Si36^{36}S, 30^{30}Si33^{33}S, 30^{30}Si36^{36}S) in its ground (X 1Σ+^1\Sigma^+) electronic state. The calculations employ an existing spectroscopically accurate potential energy curve (PEC) derived from experimental measurements and a newly-computed ab initio dipole moment curve (DMC). The 28^{28}Si32^{32}S line list includes 10104 states and 91715 transitions. These line lists are available from the ExoMol website www.exomol.com and the CDS database.

Keywords

Cite

@article{arxiv.1806.11177,
  title  = {ExoMol line lists XXV: A hot line list for silicon sulphide, SiS},
  author = {Apoorva Upadhyay and Eamon K. Conway and Jonathan Tennyson and Sergei N. Yurchenko},
  journal= {arXiv preprint arXiv:1806.11177},
  year   = {2018}
}