Energy levels, radiative rates, and excitation rates for transitions in O IV

15Citations
Citations of this article
5Readers
Mendeley users who have this article in their library.

Abstract

Aims. In this paper we report calculations for energy levels, radiative rates, and excitation rates for transitions in O IV. Methods. The GRASP (general-purpose relativistic atomic structure package) and FAC (flexible atomic code) were adopted for calculating energy levels and radiative rates, and the Dirac atomic R-matrix code (DARC) used to determine the excitation rates. Results. Oscillator strengths and radiative rates are reported for all E1, E2, M1, and M2 transitions among the lowest 75 levels of O IV. Additionally, lifetimes are reported for all levels and comparisons made with those available in the literature. Finally, effective collision strengths are reported for all transitions over a wide temperature range below 106 K. Comparisons are made with earlier results and the accuracy of the data is assessed. © ESO 2008.

Author supplied keywords

Cite

CITATION STYLE

APA

Aggarwal, K. M., & Keenan, F. P. (2008). Energy levels, radiative rates, and excitation rates for transitions in O IV. Astronomy and Astrophysics, 486(3), 1053–1067. https://doi.org/10.1051/0004-6361:20078741

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free