A core collapse supernova occurs when exothermic fusion ceases in the core of a massive star, which is typically caused by exhaustion of nuclear fuel. Theory predicts that fusion could be interrupted earlier by merging of the star with a compact binary companion. We report a luminous radio transient, VT J121001+495647, found in the Very Large Array Sky Survey. The radio emission is consistent with supernova ejecta colliding with a dense shell of material, potentially ejected by binary interaction in the centuries before explosion. We associate the supernova with an archival x-ray transient, which implies that a relativistic jet was launched during the explosion. The combination of an early relativistic jet and late-time dense interaction is consistent with expectations for a merger-driven explosion.
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Bhakta, D. ; Mooley, K. P. ; Corsi, A. ; Balasubramanian, A. ; Dobie, D. ; Frail, D. A. ; Hallinan, G. ; Kaplan, D. L. ; Myers, S. T. ; Singer, L. P. ( , The Astrophysical Journal)null (Ed.)
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Mooley, K. P. ; Nakar, E. ; Hotokezaka, K. ; Hallinan, G. ; Corsi, A. ; Frail, D. A. ; Horesh, A. ; Murphy, T. ; Lenc, E. ; Kaplan, D. L. ; et al ( , Nature)
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Hallinan, G. ; Corsi, A. ; Mooley, K. P. ; Hotokezaka, K. ; Nakar, E. ; Kasliwal, M. M. ; Kaplan, D. L. ; Frail, D. A. ; Myers, S. T. ; Murphy, T. ; et al ( , Science)
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Abbott, B. P. ; Abbott, R. ; Abbott, T. D. ; Acernese, F. ; Ackley, K. ; Adams, C. ; Adams, T. ; Addesso, P. ; Adhikari, R. X. ; Adya, V. B. ; et al ( , The Astrophysical Journal)
