A large-scale R-matrix calculation for electron-impact excitation of the Ne O-like ion
arXiv:1102.5127 · doi:10.1088/0953-4075/44/17/175206
Abstract
The five J levels within a or ground state complex provide an excellent testing ground for the comparison of theoretical line ratios with astrophysically observed values, in addition to providing valuable electron temperature and density diagnostics. The low temperature nature of the line ratios ensure that the theoretically derived values are sensitive to the underlying atomic structure and electron-impact excitation rates. Previous R-matrix calculations for the Ne O-like ion exhibit large spurious structure in the cross sections at higher electron energies, which may affect Maxwellian averaged rates even at low temperatures. Furthermore, there is an absence of comprehensive excitation data between the excited states that may provide newer diagnostics to compliment the more established lines discussed in this paper. To resolve these issues, we present both a small scale 56-level Breit-Pauli (BP) calculation and a large-scale 554 levels R-matrix Intermediate Coupling Frame Transformation (ICFT) calculation that extends the scope and validity of earlier JAJOM calculations both in terms of the atomic structure and scattering cross sections. Our results provide a comprehensive electron-impact excitation data set for all transitions to higher shells. The fundamental atomic data for this O-like ion is subsequently used within a collisional radiative framework to provide the line ratios across a range of electron temperatures and densities of interest in astrophysical observations.
arXiv comment17 pages, 8 figures
Cited by in corpus (11)
- The Galactic radial abundance gradients of C, N, O, Ne, S, Cl and Ar from deep spectra of H II regions
- Photoionized Herbig-Haro objects in the Orion Nebula through deep high-spectral resolution spectroscopy I: HH529II and III
- The homogeneity of chemical abundances in H II regions of the Magellanic Clouds
- Spitzer Infrared Spectrograph Observations of the Galactic Center: Quantifying the Extreme Ultraviolet/so ft X-ray fluxes
- Photoionized Herbig-Haro objects in the Orion Nebula through deep high-spectral resolution spectroscopy II: HH204
- Spitzer IRS Observations of the XA Region in the Cygnus Loop Supernova Remnant
- The impact of spectra quality on nebular abundances
- Spitzer observations of extragalactic H II regions - III. NGC 6822 and the hot star, H II region connection
- Fine-structure electron-impact excitation of Ne and Ne for low temperature astrophysical plasmas
- R-matrix electron-impact excitation data for the O-like iso-electronic sequence
- Beyond the [OIII]4363 auroral line: [NeIII]3868 as a direct tracer of electron temperature