H-, He-like recombination spectra III. n-changing collisions in highly-excited Rydberg states and their impact on the radio, IR and optical recombination lines

F. Guzmán, M. Chatzikos, P. A. M. van Hoof, Dana S. Balser, M. Dehghanian, N. R. Badnell, G.J. Ferland

Research output: Contribution to journalArticle

5 Citations (Scopus)
24 Downloads (Pure)

Abstract

At intermediate to high densities, electron (de-)excitation collisions are the dominant process for populating or depopulating high Rydberg states. In particular, the accurate knowledge of the energy changing (n-changing) collisional rates is determinant for predicting the radio recombination spectra of gaseous nebula. The different data sets present in the literature come either from impact parameter calculations or semi-empirical fits and the rate coefficients agree within a factor of 2. We show in this paper that these uncertainties cause errors lower than 5 per cent in the emission of radio recombination lines of most ionized plasmas of typical nebulae. However, in special circumstances where the transitions between Rydberg levels are amplified by maser effects, the errors can increase up to 20 per cent. We present simulations of the optical depth and Hnα line emission of active galactic nuclei broad-line regions and the Orion Nebula Blister to showcase our findings.

Original languageEnglish
Pages (from-to)1003–1018
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume486
Issue number1
Early online date27 Mar 2019
DOIs
Publication statusPublished - 1 Jun 2019

Keywords

  • recombination spectra
  • Rydberg states
  • electron collisions
  • radio recombination lines

Cite this