SIMBAD references

2020MNRAS.492.3794Z - Mon. Not. R. Astron. Soc., 492, 3794-3802 (2020/March-1)

Formation of CO+ by radiative association II.

ZAMECNIKOVA M., GUSTAFSSON M., NYMAN G. and SOLDAN P.

Abstract (from CDS):

Radiative association of an oxygen atom with a carbon cation is investigated using quantal and semiclassical methods. The total rate coefficient for spontaneous radiative association of O(2s22p4, 3P) with C+(2s22p, 2P) on the doublet manifold is determined from the corresponding cross-sections. The cross-sections for the 1^2 Σ ^-= A^2Π, 2^2 Σ ^-= A^2Π, and C^2 [?] = A^2Π continuum-bound processes are calculated either semiclassically, in combination with the Breit-Wigner approach, or fully quantum mechanically. In the temperature range 10-10 000 K, our recommended total rate coefficient, obtained from these calculations and the data of Zamecnikova et al. (2019), slowly increases from 7.5 x 10-18 cm3s-1 to 2.1 x 10-17 cm3s-1. Corresponding aspects of the CO+ and CO formations in SN 1987A are discussed.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): astrochemistry - molecular processes - radiation mechanisms: general - supernovae: general

Simbad objects: 3

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