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The Fast Evolution of SN 2010bh associated with GRB 100316D

Published online by Cambridge University Press:  05 September 2012

E. Felipe Olivares
Affiliation:
Max-Planck-Institute für extraterrestrische Physik, Giessenbachstraße 1, 85748, Garching, Germany, email: foe@mpe.mpg.de
Jochen Greiner
Affiliation:
Max-Planck-Institute für extraterrestrische Physik, Giessenbachstraße 1, 85748, Garching, Germany, email: foe@mpe.mpg.de
Patricia Schady
Affiliation:
Max-Planck-Institute für extraterrestrische Physik, Giessenbachstraße 1, 85748, Garching, Germany, email: foe@mpe.mpg.de
Arne Rau
Affiliation:
Max-Planck-Institute für extraterrestrische Physik, Giessenbachstraße 1, 85748, Garching, Germany, email: foe@mpe.mpg.de
Sylvio Klose
Affiliation:
Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778, Tautenburg, Germany
Thomas Krühler
Affiliation:
Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100, Copenhagen, Denmark
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Abstract

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We report on the type-Ic SN 2010bh associated with XRF 100316D at z = 0.059, which is among the latest spectroscopically confirmed GRB-SNe (Bufano et al. 2012). This supernova proves to be the most rapidly evolving GRB-SN to date.

Type
Poster Papers
Copyright
Copyright © International Astronomical Union 2012

References

Bufano, F., Pian, E., Sollerman, J., et al. 2012, ApJ submitted, arXiv:1111.4527Google Scholar
Campana, S., Mangano, V., Blustin, A. J., et al. 2006, Nature, 442, 1008CrossRefGoogle Scholar
Cano, Z., Bersier, D., Guidorzi, C., et al. 2011, ApJ, 740, 41CrossRefGoogle Scholar
Hjorth, J. & Bloom, J. S. 2011, in Gamma-Ray Bursts, ed. Kouveliotou, C., Wijers, R. A. M. J., & Woosley, S. E. (Cambridge: Cambridge Univ. Press), arXiv:1104.2274Google Scholar
Maeda, K., Mazzali, P. A., Deng, J., et al. 2003, ApJ, 593, 931CrossRefGoogle Scholar
Olivares, E. F., Greiner, J., Schady, P., et al. 2012, A&A, 539, A76Google Scholar
Starling, R. L. C., Wiersema, K., Levan, A. J., et al. 2011, MNRAS, 411, 2792CrossRefGoogle Scholar
Valenti, S., Benetti, S., Cappellaro, E., et al. 2008, MNRAS, 383, 1485CrossRefGoogle Scholar
Woosley, S. E. & Bloom, J. S. 2006, ARAA, 44, 507CrossRefGoogle Scholar
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