Formation of CO+ by radiative association II
2020 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 492, no 3, p. 3794-3802Article in journal (Refereed) Published
Abstract [en]
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 12 Σ - → A2 II, 22 Σ - → A2II, and C2 Δ → A2II 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 Zámecniková et al. (2019), slowly increases from 7.5 × 10-18 cm3s-1 to 2.1 × 10-17 cm3s-1. Corresponding aspects of the CO+ and CO formations in SN 1987A are discussed
Place, publisher, year, edition, pages
Oxford University Press, 2020. Vol. 492, no 3, p. 3794-3802
Keywords [en]
astrochemistry, molecular processes, radiation mechanisms: general, supernovae: general, ISM: molecules
National Category
Astronomy, Astrophysics and Cosmology Atom and Molecular Physics and Optics Other Physics Topics
Research subject
Applied Physics
Identifiers
URN: urn:nbn:se:ltu:diva-77537DOI: 10.1093/mnras/stz3641ISI: 000518143200052Scopus ID: 2-s2.0-85084543967OAI: oai:DiVA.org:ltu-77537DiVA, id: diva2:1388970
Note
Validerad;2020;Nivå 2;2020-02-18 (johcin)
2020-01-282020-01-282020-05-28Bibliographically approved