Article
Nature 453, 469-474 (22 May 2008) | doi:10.1038/nature06997; Received 11 February 2008; Accepted 4 April 2008
There is a Corrigendum (10 July 2008) associated with this document.
An extremely luminous X-ray outburst at the birth of a supernova
A. M. Soderberg1,2, E. Berger1,2, K. L. Page3, P. Schady4, J. Parrent5, D. Pooley6, X.-Y. Wang7, E. O. Ofek8, A. Cucchiara9, A. Rau8, E. Waxman10, J. D. Simon8, D. C.-J. Bock11, P. A. Milne12, M. J. Page4, J. C. Barentine13, S. D. Barthelmy14, A. P. Beardmore3, M. F. Bietenholz15,16, P. Brown9, A. Burrows1, D. N. Burrows9, G. Byrngelson17, S. B. Cenko18, P. Chandra19, J. R. Cummings20, D. B. Fox9, A. Gal-Yam10, N. Gehrels20, S. Immler20, M. Kasliwal8, A. K. H. Kong21, H. A. Krimm20,22, S. R. Kulkarni8, T. J. Maccarone23, P. Mészáros9, E. Nakar24, P. T. O'Brien3, R. A. Overzier25, M. de Pasquale4, J. Racusin9, N. Rea26 & D. G. York27
- Department of Astrophysical Sciences, Princeton University, Ivy Lane, Princeton, New Jersey 08544, USA
- Carnegie Observatories, 813 Santa Barbara Street, Pasadena, California 91101, USA
- Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK
- Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK
- Physics and Astronomy Department, Dartmouth College, Hanover, New Hampshire 03755, USA
- Astronomy Department, University of Wisconsin, 475 North Charter Street, Madison, Wisconsin 53706, USA
- Department of Astronomy, Nanjing University, Nanjing 210093, China
- Department of Astronomy, 105-24, California Institute of Technology, Pasadena, California 91125, USA
- Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
- Faculty of Physics, Weizmann Institute of Science, Rehovot 76100, Israel
- Radio Astronomy Laboratory, University of California, Berkeley, California 94720, USA
- Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721, USA
- Department of Astronomy, University of Texas at Austin, Austin, Texas 78712, USA
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
- Department of Physics and Astronomy, York University, Toronto, Ontario M3J 1P3, Canada
- Hartebeestehoek Radio Observatory, PO Box 443, Krugersdorp, 1740, South Africa
- Department of Physics and Astronomy, Clemson University, Clemson, South Carolina 29634, USA
- Space Radiation Laboratory, 220-47, California Institute of Technology, Pasadena, California 91125, USA
- Department of Astronomy, University of Virginia, PO Box 400325, Charlottesville, Virginia 22904, USA
- CRESST and NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
- Institute of Astronomy and Department of Physics, National Tsing Hua University, Hsinchu, Taiwan
- Universities Space Research Association, 10211 Wincopin Circle, #500, Columbia, Maryland 21044, USA
- School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
- Theoretical Astrophysics, 130-33, California Institute of Technology, Pasadena, California 91125, USA
- Max-Planck-Institut für Astrophysik, D-85748 Garching, Germany
- University of Amsterdam, Astronomical Institute 'Anton Pannekoek', Kruislaan 403, 1098SJ, Amsterdam, The Netherlands
- Department of Astronomy and Astrophysics, University of Chicago, 5640 S. Ellis Avenue, Chicago, Illinois 60637, USA
Correspondence to: A. M. Soderberg1,2 Correspondence and requests for materials should be addressed to A.M.S. (Email: alicia@astro.princeton.edu).
Abstract
Massive stars end their short lives in spectacular explosions—supernovae—that synthesize new elements and drive galaxy evolution. Historically, supernovae were discovered mainly through their 'delayed' optical light (some days after the burst of neutrinos that marks the actual event), preventing observations in the first moments following the explosion. As a result, the progenitors of some supernovae and the events leading up to their violent demise remain intensely debated. Here we report the serendipitous discovery of a supernova at the time of the explosion, marked by an extremely luminous X-ray outburst. We attribute the outburst to the 'break-out' of the supernova shock wave from the progenitor star, and show that the inferred rate of such events agrees with that of all core-collapse supernovae. We predict that future wide-field X-ray surveys will catch each year hundreds of supernovae in the act of exploding.
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