Multi-Zone Models of Superbursts from Accreting Neutron Stars
SN 2010ay is a Luminous and Broad-lined Type Ic Supernova within a Low-metallicity Host Galaxy
- Authors: Nathan E. Sanders (1), A. M. Soderberg (1), S. Valenti (2), L. Chomiuk (1,3), E. Berger (1), S. Smartt (2), K. Hurley (4), S. D. Barthelmy (5), R. Chornock (1), R. J. Foley (1), E. M. Levesque (6), G. Narayan (7), R. P. Kirshner (1), M.T. Botticella (2), M. S. Briggs (8), V. Connaughton (8), Y. Terada (9), N. Gehrels (5), S. Golenetskii (10), E. Mazets (10), T. Cline (11), A. von Kienlin (12), W. Boynton (13), K. C. Chambers (14), T. Grav (15), J. N. Heasley (14), K. W. Hodapp (14), R. Jedicke (14), N. Kaiser (14), R.-P. Kudritzki (14), G. A. Luppino (14), R. H. Lupton (16), E. A. Magnier (14), D. G. Monet (17), J. S. Morgan (14), P. M. Onaka (14), P. A. Price (14), C. W. Stubbs (7), J. L. Tonry (14), R. J. Wainscoat (14), M. F. Waterson (18) ((1) Harvard-Smithsonian Center for Astrophysics, (2) Queens University, (3) National Radio Astronomy Observatory, (4) University of California Berkeley, (5) NASA Goddard Space Flight Center, (6) University of Colorado, (7) Department of Physics, Harvard University, (8) CSPAR, University of Alabama in Huntsville, (9) Saitama University, (10) Ioffe Physico-Technical Institute, (11) Emeritus, NASA Goddard Space Flight Center, (12) Max-Planck Institut fur extraterrestrische Physik, Garching, (13) Lunar and Planetary Laboratory, University of Arizona, (14) Institute for Astronomy, University of Hawaii, (15) Johns Hopkins University, Baltimore, MD, USA, (16) Princeton University, (17) US Naval Observatory, Flagstaff Station, (18) The University of Western Australia)
Charged Particle Decay at Finite Temperature
Probing Superluminal Neutrinos Via Refraction