SIMBAD references

2018MNRAS.479.3227D - Mon. Not. R. Astron. Soc., 479, 3227-3231 (2018/September-3)

Hyperfine excitation of C2H in collisions with ortho- and para-H2.

DAGDIGIAN P.J.

Abstract (from CDS):

Accurate estimation of the abundance of the ethynyl (C2H) radical requires accurate radiative and collisional rate coefficients. Hyperfine-resolved rate coefficients for (de-)excitation of C2H in collisions with ortho- and para-H2 are presented in this work. These rate coefficients were computed in time-independent close-coupling quantum scattering calculations that employed a potential energy surface recently computed at the coupled-clusters level of theory that describes the interaction of C2H with H2. Rate coefficients for temperatures from 10 to 300 K were computed for all transitions among the first 40 hyperfine energy levels of C2H in collisions with ortho- and para-H2. These rate coefficients were employed in simple radiative transfer calculations to simulate the excitation of C2H in typical molecular clouds.

Abstract Copyright: © 2018 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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