Abstract

For pt.I see ibid., vol.18, p.1589 (1985). Formulae obtained by Bell and Seaton in the first paper of the present series are used to calculate collision strengths for the 1 1S-21S transitions in O6+ at energies below the 21P threshold. Radiative decays lead to modifications of autoionising resonance profiles and substantial reductions in collision strengths averaged over resonances.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.