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Binary Stars Can Provide the "Missing Photons" Needed for Reionization

, , , , , , and . (2016)cite arxiv:1601.07559Comment: 6 pages, 3 figures, submitted to MNRAS Letter.

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Pair-Instability Supernovae at the Epoch of Reionization, , and . (2011)cite arxiv:1112.2710Comment: 12 pages, 11 figures. Submitted to MNRAS. arXiv admin note: some text overlap with arXiv:0809.3926.The Diversity of Transients from Magnetar Birth, , , and . (Aug 11, 2015)Astrophysics: The supernova has two faces. Nature, 466 (7302): 37--38 (July 2010)Discrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf Galaxies, , , , , , , , and . (2017)cite arxiv:1712.02795Comment: 9 pages, 4 figures.Pair-Instability Supernovae via Collision Runaway in Young Dense Star Clusters, , and . (2011)cite arxiv:1111.3648Comment: 5 pages, 4 figures.Binary Stars Can Provide the "Missing Photons" Needed for Reionization, , , , , , and . (2016)cite arxiv:1601.07559Comment: 6 pages, 3 figures, submitted to MNRAS Letter.The Difficulty Getting High Escape Fractions of Ionizing Photons from High-redshift Galaxies: a View from the FIRE Cosmological Simulations, , , , , , and . (2015)cite arxiv:1503.07880Comment: 16 pages, 14 figures, submitted to MNRAS; comments welcome.Supernova signals of light dark matter, , , , and . (2019)cite arxiv:1905.09284Comment: 33 pages, 8 figures.Atomic Chemistry In Turbulent Astrophysical Media I: Effect of Atomic Cooling. (2015)cite arxiv:1502.01019Comment: 17 Pages, 8 figures, Accepted to ApJ. Comments welcome.