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What can produce a sharp late time optical re‐brightening? Optical bumps in the multi‐color imaging era

MPS-Authors
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Nardini,  M.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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

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

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Filgas,  R.
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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Afonso,  P.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Clemens,  C.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Olivares,  F. E.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Burlon,  D.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Citation

Nardini, M., Greiner, J., Klose, S., Krühler, T., Filgas, R., Schady, P., et al. (2011). What can produce a sharp late time optical re‐brightening? Optical bumps in the multi‐color imaging era. In J. E. McEnery, J. L. Racusin, & N. Gehrels (Eds.), Gamma Ray Bursts 2010 (pp. 150-153).


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-46D4-B
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