2018MNRAS.481.1858P


Query : 2018MNRAS.481.1858P

2018MNRAS.481.1858P - Mon. Not. R. Astron. Soc., 481, 1858-1861 (2018/December-1)

Accurate theoretical predictions on the mechanisms of OSiS formation and its dissociation channels.

PAIVA M.A.M., LEFLOCH B. and GALVAO B.R.L.

Abstract (from CDS):

Multireference configuration interaction calculations are performed to investigate the potential energy surface of the S+SiO and O+SiS reactions, which are of astrochemical relevance. Several singlet and triplet electronic states are calculated in order to explore the reaction paths. It is shown that although collisions with ground-state reactants do not lead to the OSiS molecule adiabatically, the probabilities for such a spin-forbidden process are high. It is also predicted that SiS is easily converted to SiO. Spin orbit couplings and other properties are also calculated and several electronic states are explored.

Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): astrochemistry - molecular data - ISM: molecules

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Orion-KL SFR 05 35 14.16 -05 22 21.5           ~ 2421 1
2 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 2443 1
3 [DE95] LDN 1157 B1 out 20 39 11 +68 01.3           ~ 288 0

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