Stark Broadening of Cr III Spectral Lines: DO White Dwarfs
Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia
LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universities, UPMC, Paris 06, 5 Place Jules Janssen, 92195 Meudon CEDEX, France
Institut für Astro- und Teilchenphysik, Universität Innsbruck, Technikerstr. 25/8, A-6020 Innsbruck, Austria
Author to whom correspondence should be addressed.
Current address: Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia.
Received: 7 March 2018 / Revised: 24 March 2018 / Accepted: 26 March 2018 / Published: 3 April 2018
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Using the modified semiempirical method of Dimitrijević and Konjević, Stark widths have been calculated for six Cr III transitions, for an electron density of 10
and for temperatures from 5000–80,000 K. Results have been used for the investigation of the influence of Stark broadening on spectral lines in cool DO white dwarf atmospheres. Calculated Stark widths will be implemented in the STARK-B database, which is also a part of the Virtual Atomic and Molecular Data Center (VAMDC).
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MDPI and ACS Style
Dimitrijević, M.S.; Chougule, A. Stark Broadening of Cr III Spectral Lines: DO White Dwarfs. Atoms 2018, 6, 15.
Dimitrijević MS, Chougule A. Stark Broadening of Cr III Spectral Lines: DO White Dwarfs. Atoms. 2018; 6(2):15.
Dimitrijević, Milan S.; Chougule, Abhishek. 2018. "Stark Broadening of Cr III Spectral Lines: DO White Dwarfs." Atoms 6, no. 2: 15.
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