JINA - Virtual Journal of Nuclear Astrophysics,
26 January 2018
Volume 16, Issue 4 (46 Articles)
- # 2 - Alternative explanations for extreme supersolar iron abundances inferred from the energy spectrum of Cygnus X-1. (arXiv:1801.07267v1 [astro-ph.HE])
- John A. Tomsick (SSL/UCB), Michael L. Parker (ESAC), Javier A. Garcia (Caltech, Univ. Erlangen-Nurnberg), Kazutaka Yamaoka (Nagoya Univ.), Didier Barret (Univ. de Toulouse, CNRS), Jeng-Lun Chiu (National Tsing Hua Univ.), Maica Clavel (SSL/UCB, Univ. Grenoble Alpes), Andrew Fabian (Cambridge), Felix Furst (ESAC), Poshak Gandhi (Univ. of Southampton), Victoria Grinberg (ESTEC), Jon M. Miller (Univ. of Michigan), Katja Pottschmidt (NASA/GSFC, Univ. of Maryland), Dominic J. Walton (Cambridge)
- http://arxiv.org/abs/1801.07267
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.
