Stellar laboratories: IX. New Se v, Sr iv-vii, Te vi, and I vi oscillator strengths and the Se, Sr, Te, and I abundances in the hot white dwarfs G191−B2B and RE 0503−289
<i>Context. <i/>To analyze spectra of hot stars, advanced non-local thermodynamic equilibrium (NLTE) model-atmosphere techniques are mandatory. Reliable atomic data is crucial for the calculation of such model atmospheres. <i>Aims. <i/>We aim to calculate new Sr iv-vii oscill...
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
20 October 2017
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| In: |
Astronomy and astrophysics
Year: 2017, Jahrgang: 606 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201730383 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201730383 Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2017/10/aa30383-17/aa30383-17.html 
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| Verfasserangaben: | T. Rauch, P. Quinet, M. Knörzer, D. Hoyer, K. Werner, J. W. Kruk, and M. Demleitner |
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Stellar laboratories: IX. New Se V, Sr IV - VII, Te VI, and I VI oscillator strengths and the Se, Sr, Te, and I abundances in the hot white dwarfs G191-B2B and RE 0503-289
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