2019MNRAS.487.3427D


Query : 2019MNRAS.487.3427D

2019MNRAS.487.3427D - Mon. Not. R. Astron. Soc., 487, 3427-3431 (2019/August-2)

Hyperfine excitation of SH+ in collisions with para- and ortho-H2.

DAGDIGIAN P.J.

Abstract (from CDS):

Time-independent close-coupling quantum scattering calculations are employed to compute hyperfine-resolved rate coefficients for (de-)excitation of SH+ in collisions with para- and ortho-H2. These calculations utilized a potential energy surface for the interaction of SH+(X3Σ–) with H2 recently computed by the explicitly correlated RCCSD(T)-F12a coupled-cluster method. Rate coefficients for temperatures ranging from 10 to 500 K were calculated for all transitions among the first 37 hyperfine energy levels of SH+, with rotational angular momenta n <= 6, in collisions with para- and ortho-H2. As a first application of these data, the rate coefficients were employed in simple radiative transfer calculations to simulate the excitation of SH+ in typical molecular clouds.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): molecular data - molecular processes - ISM : abundances

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 W3 IRS 5 Y*O 02 25 40.54 +62 05 51.4           B1 367 0
2 NAME Orion Bright Bar reg 05 35 22.30 -05 24 33.0           ~ 1004 0
3 NAME Sgr B2 Main Rad 17 47 20.5 -28 23 06           ~ 436 1

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