期刊
NATURE
卷 523, 期 7559, 页码 189-U316出版社
NATURE PUBLISHING GROUP
DOI: 10.1038/nature14579
关键词
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资金
- DFG cluster of excellence Origin and Structure of the Universe
- Alexander von Humboldt Foundation, Germany
- EXTraS from the European Union
- DFG
- Thuringer Ministerium fur Bildung, Wissenschaft und Kultur
- FONDECYT
- Czech MEYS
- Leibniz-Prize
- DNRF
- STFC [ST/L00061X/1] Funding Source: UKRI
- Science and Technology Facilities Council [1507817, ST/L00061X/1] Funding Source: researchfish
A new class of ultra-long-duration (more than 10,000 seconds) gamma-ray bursts has recently been suggested(1-3). They may originate in the explosion of stars with much larger radii than those producing normal long-duration gamma-ray bursts(3,4) or in the tidal disruption of a star(3). No clear supernova has yet been associated with an ultra-long-duration gamma-ray burst. Here we report that a supernova (SN 2011kl) was associated with the ultra-long-duration gamma-ray burst GRB 111209A, at a redshift z of 0.677. This supernova is more than three times more luminous than type Ic supernovae associated with long-duration gamma-ray bursts(5-7), and its spectrum is distinctly different. The slope of the continuum resembles those of super-luminous supernovae(8,9), but extends further down into the rest-frame ultraviolet implying a low metal content. The light curve evolves much more rapidly than those of super-luminous supernovae. This combination of high luminosity and low metalline opacity cannot be reconciled with typical type Ic supernovae, but can be reproduced by a model where extra energy is injected by a strongly magnetized neutron star (a magnetar), which has also been proposed as the explanation for super-luminous supernovae(10).
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