Stark Broadening of the Spectral Lines of Ne v

Abstract

Using a semiclassical approach, we have calculated ab initio electron-, proton-, and ionized helium-impact line widths and shift for 26 Ne v multiplets. Energy levels and oscillator strengths have been calculated using SUPERSTRUCTURE code. Results have been presented for an electron density of 10 17 cm -3 as a function of temperature, and are compared with experimental and other theoretical results. © 2007. The American Astronomical Society. All rights reserved.