Author
Listed:
- M. C. Bersten
(Instituto de Astrofísica de La Plata (IALP)
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque
Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, University of Tokyo)
- G. Folatelli
(Instituto de Astrofísica de La Plata (IALP)
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque
Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, University of Tokyo)
- F. García
(Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque
Instituto Argentino de Radioastronomía (CCT-La Plata, CONICET
CICPBA)
Université Paris Diderot, AIM, Sorbonne Paris Cité, CEA)
- S. D. Van Dyk
(Caltech/IPAC)
- O. G. Benvenuto
(Instituto de Astrofísica de La Plata (IALP)
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque)
- M. Orellana
(Sede Andina, Universidad Nacional de Río Negro)
- V. Buso
(Observatorio Astronómico Busoniano)
- J. L. Sánchez
(Observatorio Astronómico Geminis Austral)
- M. Tanaka
(National Astronomical Observatory of Japan, National Institutes of Natural Sciences)
- K. Maeda
(Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, University of Tokyo
Kyoto University, Kitashirakawa-Oiwake-cho)
- A. V. Filippenko
(University of California
Miller Senior Fellow, Miller Institute for Basic Research in Science, University of California)
- W. Zheng
(University of California)
- T. G. Brink
(University of California)
- S. B. Cenko
(NASA Goddard Space Flight Center
Joint Space-Science Institute, University of Maryland)
- T. de Jaeger
(University of California)
- S. Kumar
(Florida State University)
- T. J. Moriya
(National Astronomical Observatory of Japan, National Institutes of Natural Sciences)
- K. Nomoto
(Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, University of Tokyo)
- D. A. Perley
(Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park)
- I. Shivvers
(University of California)
- N. Smith
(Steward Observatory, University of Arizona)
Abstract
The discovery of a newly born type IIb supernova reveals a rapid brightening at optical wavelengths that corresponds to the shock-breakout phase of the explosion.
Suggested Citation
M. C. Bersten & G. Folatelli & F. García & S. D. Van Dyk & O. G. Benvenuto & M. Orellana & V. Buso & J. L. Sánchez & M. Tanaka & K. Maeda & A. V. Filippenko & W. Zheng & T. G. Brink & S. B. Cenko & T., 2018.
"A surge of light at the birth of a supernova,"
Nature, Nature, vol. 554(7693), pages 497-499, February.
Handle:
RePEc:nat:nature:v:554:y:2018:i:7693:d:10.1038_nature25151
DOI: 10.1038/nature25151
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