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

X. Ma, P. Hopkins, D. Kasen, E. Quataert, C. Faucher-Giguere, D. Keres, и N. Murray. (2016)cite arxiv:1601.07559Comment: 6 pages, 3 figures, submitted to MNRAS Letter.

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Paul Kasenbacher

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The Diversity of Transients from Magnetar BirthB. Metzger, B. Margalit, D. Kasen, и E. Quataert. (11.08.2015)Pair-Instability Supernovae at the Epoch of ReionizationT. Pan, D. Kasen, и A. Loeb. (2011)cite arxiv:1112.2710Comment: 12 pages, 11 figures. Submitted to MNRAS. arXiv admin note: some text overlap with arXiv:0809.3926.Discrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf GalaxiesK. Su, P. Hopkins, C. Hayward, X. Ma, M. Boylan-Kolchin, D. Kasen, D. Kereš, C. Faucher-Giguère, и M. Orr. (2017)cite arxiv:1712.02795Comment: 9 pages, 4 figures.Pair-Instability Supernovae via Collision Runaway in Young Dense Star ClustersT. Pan, A. Loeb, и D. Kasen. (2011)cite arxiv:1111.3648Comment: 5 pages, 4 figures.Astrophysics: The supernova has two facesD. Kasen. Nature, 466 (7302): 37--38 (июля 2010)Exascale models of stellar explosions: Quintessential multi-physics simulation.J. Harris, R. Chu, S. Couch, A. Dubey, E. Endeve, A. Georgiadou, R. Jain, D. Kasen, M. Laiu, O. Messer и 3 other автор(ы). Int. J. High Perform. Comput. Appl., 36 (1): 59-77 (2022)The Difficulty Getting High Escape Fractions of Ionizing Photons from High-redshift Galaxies: a View from the FIRE Cosmological SimulationsX. Ma, D. Kasen, P. Hopkins, C. Faucher-Giguere, E. Quataert, D. Keres, и N. Murray. (2015)cite arxiv:1503.07880Comment: 16 pages, 14 figures, submitted to MNRAS; comments welcome.Binary Stars Can Provide the "Missing Photons" Needed for ReionizationX. Ma, P. Hopkins, D. Kasen, E. Quataert, C. Faucher-Giguere, D. Keres, и N. Murray. (2016)cite arxiv:1601.07559Comment: 6 pages, 3 figures, submitted to MNRAS Letter.Supernova signals of light dark matterW. DeRocco, P. Graham, D. Kasen, G. Marques-Tavares, и S. Rajendran. (2019)cite arxiv:1905.09284Comment: 33 pages, 8 figures.Atomic Chemistry In Turbulent Astrophysical Media I: Effect of Atomic CoolingW. Kasen. (2015)cite arxiv:1502.01019Comment: 17 Pages, 8 figures, Accepted to ApJ. Comments welcome.

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