Unified line profiles for hydrogen perturbed by collisions with protons: satellites and asymmetries
arXiv:1501.05609 · doi:10.1093/mnras/stv167
Abstract
We present new calculations of unified line profiles for hydrogen perturbed by collisions with protons. We report on new calculations of the potential energies and dipole moments which allow the evaluation of profiles for the lines of the Lyman series up to Lyman and the Balmer series up to Balmer10. Unified calculations only existed for the lines Lyman to Lyman and Balmer including the H quasi-molecule. These data are available as online material accompanying this paper and should be included in atmosphere models, in place of the Stark effect of protons, since the quasi-molecular contributions cause not only satellites, but large asymmetries that are unaccounted for in models that assume Stark broadening of electrons and protons are equal.
13 pages, 25 figures. Accepted for publication in MNRAS
References in corpus (7)
- Found: The missing blue opacity in atmosphere models of cool hydrogen white dwarfs
- Super and massive AGB stars - IV. Final fates - Initial to final mass relation
- New white dwarf stars in the Sloan Digital Sky Survey Data Release 10
- White Dwarf Cosmochronology in the Solar Neighborhood
- Comparison of Atmospheric Parameters Determined from Spectroscopy and Photometry for DA White Dwarfs in the Sloan Digital Sky Survey
- Gemini spectra of 12000K white dwarf stars
- Which Hydrogen Balmer Lines Are Most Reliable for Determining White Dwarf Atmospheric Parameters?