Stellar laboratories: VIII. New Zr IV - VII, Xe IV - V, and Xe VII oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs G191-B2B and RE0503-289
<i>Context. <i/>For the spectral analysis of high-resolution and high-signal-to-noise spectra of hot stars, state-of-the-art non-local thermodynamic equilibrium (NLTE) model atmospheres are mandatory. These are strongly dependent on the reliability of the atomic data that is used for the...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
16 March 2017
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| In: |
Astronomy and astrophysics
Year: 2017, Volume: 599 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201629794 |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201629794
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| Author Notes: | T. Rauch, S. Gamrath, P. Quinet, L. Löbling, D. Hoyer, K. Werner, J.W. Kruk, and M. Demleitner |
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Stellar laboratories: VIII. New Zr IV - VII, Xe IV - V, and Xe VII oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs G191-B2B and RE0503-289
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