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A kilonova as the electromagnetic counterpart to a gravitational-wave source

MPS-Authors
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Chen,  T.-W.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Jerkstrand,  A.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Krühler,  T.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Flörs,  A.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Greiner,  J.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Rau,  A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Schady,  P.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Schweyer,  T.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Taubenberger,  S.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Wiseman,  P.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Smartt, S. J., Chen, T.-W., Jerkstrand, A., Coughlin, M., Kankare, E., Sim, S. A., et al. (2017). A kilonova as the electromagnetic counterpart to a gravitational-wave source. Nature, 551(7678), 75-79. doi:10.1038/nature24303.


Cite as: http://hdl.handle.net/11858/00-001M-0000-002E-31B2-E
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