Confined dense circumstellar material surrounding a regular type II supernova
Confined dense circumstellar material surrounding a regular type II supernova
With the advent of new wide-field, high-cadence optical transient
surveys, our understanding of the diversity of core-collapse supernovae
has grown tremendously in the last decade. However, the pre-supernova
evolution of massive stars, which sets the physical backdrop to these
violent events, is theoretically not well understood and difficult to
probe observationally. Here we report the discovery of the supernova
iPTF 13dqy = SN 2013fs a mere ~3 h after explosion. Our rapid follow-up
observations, which include multiwavelength photometry and extremely
early (beginning at ~6 h post-explosion) spectra, map the distribution
of material in the immediate environment (
510-517
Yaron, O.
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Perley, D.A.
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Gal-Yam, A.
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Groh, J.H.
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Horesh, A.
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Ofek, E.O.
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Kulkarni, S.R.
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Sollerman, J.
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Fransson, C.
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Valenti, S.
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Arcavi, I.
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Howell, D.A.
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Kasliwal, M.M.
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Vreeswijk, P.M.
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Khazov, D.
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Cao, Y.
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Kelly, P.L.
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Yaron, O.
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Perley, D.A.
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Gal-Yam, A.
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Groh, J.H.
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Horesh, A.
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Ofek, E.O.
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Sollerman, J.
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Fransson, C.
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Szabo, P.
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Valenti, S.
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Arcavi, I.
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Howell, D.A.
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Kasliwal, M.M.
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Vreeswijk, P.M.
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Khazov, D.
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Cao, Y.
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Gnat, O.
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Kelly, P.L.
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Nugent, P.E.
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Filippenko, A.V.
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Laher, R.R.
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Wozniak, P.R.
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Rebbapragada, U.D.
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Maguire, K.
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Sullivan, M.
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