Data for the broadening of 24188 Fe II lines by collisions with neutral hydrogen atoms have been computed using the theory of Anstee & O'Mara as extended to singly ionised species and higher orbital angular momentum states by Barklem & O'Mara. Data have been computed for all Fe II lines between observed energy levels in the line lists of Kurucz with $\log gf > -5$ for which the theory is applicable. The variable energy debt parameter Ep used in computing the second order perturbation theory potential is chosen to be consistent with the long range dispersion interaction constant C6 computed using the f-values from Kurucz
“Stark broadening” theory and calculations have been extensively developed for about 50 years. The t...
We describe, and present the results of, a new large-scale R-matrix scattering calculation for the e...
For the first time broadening by both resonance and dispersive-inductive interactions with H-atoms a...
Data for the broadening of 24188 Fe II lines by collisions with neutral hydrogen atoms have been com...
A list of data for the broadening by neutral hydrogen collisions of many astrophysically important s...
The theory of Anstee & O'Mara for the broadening of spectral lines owing to collisions by neutral hy...
The collisional broadening theory of Anstee & O'Mara for s-p and p-s transitions by collisions with ...
The object of this thesis is to extend the current tables for two useful quantities when calculating...
Line broadening cross sections for the broadening of spectral lines by collisions with neutral hydro...
International audienceThis paper compares different approaches used in the calculation of the broade...
International audienceStark broadening parameters, full widths at half intensity maximum and shifts ...
Analyzing stellar spectra plays a big role in understanding the evolution of our galaxy. Having good...
International audienceContext: Profiles of hydrogen lines in stellar spectra are determined by the p...
Context.Profiles of hydrogen lines in stellar spectra are determined by the properties of the hydro...
We present new calculations of unified line profiles for hydrogen perturbed by collisions with proto...
“Stark broadening” theory and calculations have been extensively developed for about 50 years. The t...
We describe, and present the results of, a new large-scale R-matrix scattering calculation for the e...
For the first time broadening by both resonance and dispersive-inductive interactions with H-atoms a...
Data for the broadening of 24188 Fe II lines by collisions with neutral hydrogen atoms have been com...
A list of data for the broadening by neutral hydrogen collisions of many astrophysically important s...
The theory of Anstee & O'Mara for the broadening of spectral lines owing to collisions by neutral hy...
The collisional broadening theory of Anstee & O'Mara for s-p and p-s transitions by collisions with ...
The object of this thesis is to extend the current tables for two useful quantities when calculating...
Line broadening cross sections for the broadening of spectral lines by collisions with neutral hydro...
International audienceThis paper compares different approaches used in the calculation of the broade...
International audienceStark broadening parameters, full widths at half intensity maximum and shifts ...
Analyzing stellar spectra plays a big role in understanding the evolution of our galaxy. Having good...
International audienceContext: Profiles of hydrogen lines in stellar spectra are determined by the p...
Context.Profiles of hydrogen lines in stellar spectra are determined by the properties of the hydro...
We present new calculations of unified line profiles for hydrogen perturbed by collisions with proto...
“Stark broadening” theory and calculations have been extensively developed for about 50 years. The t...
We describe, and present the results of, a new large-scale R-matrix scattering calculation for the e...
For the first time broadening by both resonance and dispersive-inductive interactions with H-atoms a...