2022MNRAS.513.6152K


Query : 2022MNRAS.513.6152K

2022MNRAS.513.6152K - Mon. Not. R. Astron. Soc., 513, 6152-6157 (2022/July-2)

New de-excitation rates of the open shell dicarbon monoxide C2O(X3 Σ–) in collision with He(1S).

KHADRI F., HACHANI L., ELABIDI H. and HAMMAMI K.

Abstract (from CDS):

In order to derive accurate physical conditions of the interstellar clouds (such as TMC-1) from the rotational transitions of C2O, collisional rates are needed. Based on a new two-dimensional potential energy surface (PES), we report a new rate coefficients calculation of C2O(X3Σ–) induced by collision with He. This PES was obtained from the explicitly correlated restricted open-shell coupled cluster with single, double, and perturbative triple excitation (rccsd(t)-f12) ab initio approach associated with aug-cc-pVTZ basis sets. The C2O-He PES presents one minimum below its dissociation limit with a well depth of 42.376 cm–1. The close-coupling quantum time-independent formalism was used to derive cross sections for E <= 370 cm–1 and N <= 10. De-excitation rate coefficients are obtained for thermal temperature below 80 K.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): molecular data - radiative transfer - scattering - ISM: molecules

Simbad objects: 1

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Number of rows : 1
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 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0

Query : 2022MNRAS.513.6152K

Basic data :
TMC-1 -- Molecular Cloud
Other object types:
otypes_help
PoC (MLB,[MOH94]), MoC (TMC), Cld (HCL)
ICRS coord. (ep=J2000) :
04 41 45.9 +25 41 27 [ ] D 1983ApJ...264..517M
FK4 coord. (ep=B1950 eq=1950) :
04 38 42.0 +25 35 45 [ ]
Gal coord. (ep=J2000) :
174.3852 -13.4312 [ ]
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Hierarchy : number of linked objects
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Identifiers (4) :
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HCL 2 MLB 3-28 TMC-1 [MOH94] 6

References (1872 between 1850 and 2026) (Total 1872)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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