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2015MNRAS.449.2974S - Mon. Not. R. Astron. Soc., 449, 2974-2979 (2015/May-3)

Effective collision strengths for excitation and de-excitation of nebular [OIII] optical and infrared lines with κ distributed electron energies.

STOREY P.J. and SOCHI T.

Abstract (from CDS):

We present effective collision strengths for electron excitation and de-excitation of the 10 forbidden transitions between the five lowest energy levels of the astronomically abundant doubly ionized oxygen ion, O2+. The raw collision strength data were obtained from an R-matrix intermediate coupling calculation using the Breit-Pauli relativistic approximation published previously by the authors. The effective collision strengths were calculated with κ-distributed electron energies and are tabulated as a function of the electron temperature and κ.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): atomic data - atomic processes - radiation mechanisms: non-thermal - planetary nebulae: general - infrared: general

VizieR on-line data: <CDS Catalogue: VI/144>

Simbad objects: 1

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