JINA - Virtual Journal of Nuclear Astrophysics,
30 June 2017
Volume 15, Issue 26 (29 Articles)
- # 10 - 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. (arXiv:1706.09215v1 [astro-ph.SR])
- T. Rauch (1), P. Quinet (2, 3), M. Knoerzer (1), D. Hoyer (1), K. Werner (1), J. W. Kruk (5), M. Demleitner (6) ((1) Institute for Astronomy, Astrophysics, Eberhard Karls University, Tuebingen, Germany, (2) Physique Atomique et Astrophysique, Universite de Mons - UMONS, Belgium, (3) IPNAS, Universite de Liege, Liege, Belgium, (4) Institute of Physics, Astronomy, University of Potsdam, Golm, Germany, (5) NASA Goddard Space Flight Center, Greenbelt, USA, (6) Astronomisches Rechen-Institut (ARI), Centre for Astronomy of Heidelberg University, Heidelberg, Germany)
- http://arxiv.org/abs/1706.09215
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.
