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.
arXiv comment13 pages, 25 figures. Accepted for publication in MNRAS
References in corpus (23)
- The Formation Rate, Mass and Luminosity Functions of DA White Dwarfs from the Palomar Green Survey
- SDSS DR7 White Dwarf Catalog
- Spectroscopic Analysis of DA White Dwarfs: Stark Broadening of Hydrogen Lines Including Non-Ideal Effects
- A Spectroscopic Survey & Analysis of Bright, Hydrogen-Rich White Dwarfs
- 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
- Know Your Neighborhood: A Detailed Model Atmosphere Analysis of Nearby White Dwarfs
- Spectroscopic analysis of DA white dwarfs with 3D model atmospheres
- Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models
- A Gravitational Redshift Determination of the Mean Mass of White Dwarfs. DA Stars
- 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
- Lyman-alpha wing absorption in cool white dwarf stars
- An Experimental Platform for Creating White Dwarf Photospheres in the Laboratory
- FUSE observations of hot white dwarfs
- Gemini spectra of 12000K white dwarf stars
- Quasi-molecular Satellites of Lyman Beta in the Spectrum of the DA White Dwarf WOLF 1346
- A collision-induced satellite in the Lyman Beta profile due to H-H collisions
- Theoretical study of the line profiles of the hydrogen perturbed by collisions with protons
- Common Proper Motion Wide White Dwarf Binaries Selected From The Sloan Digital Sky Survey
- White Dwarfs in Globular Clusters
- Which Hydrogen Balmer Lines Are Most Reliable for Determining White Dwarf Atmospheric Parameters?