J/A+AS/113/579 J/A+AS/113/579 Stark broadening T Schoening Astron. Astrophys. Suppl. Ser. 113 579 1995 1995A&AS..113..579S atomic data line: profiles plasmas stars: abundances Tables of Stark broadening profiles for the N V 6f, g, h-7f, g, h, i line complex at 4945A have been generated. Modern close-coupling techniques are used for the electron broadening while the important influence of perturbing ions is included within the framework of the model microfield method. Comparison has been made with the results of line formation calculations using approximate formulae for the Stark profiles.

Ne Electron density cm-3 DeltaLambda0 Wavelength of intensity maximum number=1 Delta lambda = Delta lambda0 + delta lambda where Delta lambda denotes the wavelength detuning from line centre (6h-7i at 494.5 nm), Delta lambda0 the wavelength separation (relative to the line centre) of prominent intensity maxima and delta lambda the detuning from the nearest intensity maximum. 0.1nm deltaLambda Detuning from intensity maximum number=1 Delta lambda = Delta lambda0 + delta lambda where Delta lambda denotes the wavelength detuning from line centre (6h-7i at 494.5 nm), Delta lambda0 the wavelength separation (relative to the line centre) of prominent intensity maxima and delta lambda the detuning from the nearest intensity maximum. 0.1nm S2 Intensity (Temperature T= 2.10+4 K) number=2 Normalized intensity in frequency units, e- and H+ perturbers (with thermal Doppler broadening and radiative damping). Hz-1 S4 Intensity (Temperature T= 4.10+4 K) number=2 Normalized intensity in frequency units, e- and H+ perturbers (with thermal Doppler broadening and radiative damping). Hz-1 S8 Intensity (Temperature T= 8.10+4 K) number=2 Normalized intensity in frequency units, e- and H+ perturbers (with thermal Doppler broadening and radiative damping). Hz-1 S16 Intensity (Temperature T= 16.10+4 K) number=2 Normalized intensity in frequency units, e- and H+ perturbers (with thermal Doppler broadening and radiative damping). Hz-1 Ne Electron density cm-3 DeltaLambda0 Wavelength of intensity maximum number=1 Delta lambda = Delta lambda0 + delta lambda where Delta lambda denotes the wavelength detuning from line centre (6h-7i at 494.5 nm), Delta lambda0 the wavelength separation (relative to the line centre) of prominent intensity maxima and delta lambda the detuning from the nearest intensity maximum. 0.1nm deltaLambda Detuning from intensity maximum number=1 Delta lambda = Delta lambda0 + delta lambda where Delta lambda denotes the wavelength detuning from line centre (6h-7i at 494.5 nm), Delta lambda0 the wavelength separation (relative to the line centre) of prominent intensity maxima and delta lambda the detuning from the nearest intensity maximum. 0.1nm F2 Intensity (Temperature T= 2.10+4K) number=2 Normalized intensity in wavelength units, e- and H+ perturbers (Stark only). 10/nm F4 Intensity (Temperature T= 4.10+4K) number=2 Normalized intensity in wavelength units, e- and H+ perturbers (Stark only). 10/nm F8 Intensity (Temperature T= 8.10+4K) number=2 Normalized intensity in wavelength units, e- and H+ perturbers (Stark only). 10/nm F16 Intensity (Temperature T= 16.10+4K) number=2 Normalized intensity in wavelength units, e- and H+ perturbers (Stark only). 10/nm Thomas Schoening, Simona Mei CDS 1995Jun08Schoening T., <uh102ac@usm.uni-muenchen.de> J_A+AS_113_579.xml