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26 April 2024
 
  » arxiv » 1509.3279

 Article overview



A very luminous magnetar-powered supernova associated with an ultra-long gamma-ray burst
Jochen Greiner ; Paolo A. Mazzali ; D. Alexander Kann ; Thomas Krühler ; Elena Pian ; Simon Prentice ; Felipe Olivares E. ; Andrea Rossi ; Sylvio Klose ; Stefan Taubenberger ; Fabian Knust ; Paulo M.J. Afonso ; Chris Ashall ; Jan Bolmer ; Corentin Delvaux ; Roland Diehl ; Jonathan Elliott ; Robert Filgas ; Johan P.U. Fynbo ; John F. Graham ; Ana Nicuesa Guelbenzu ; Shiho Kobayashi ; Giorgos Leloudas ; Sandra Savaglio ; Patricia Schady ; Sebastian Schmid ; Tassilo Schweyer ; Vladimir Sudilovsky ; Mohit Tanga ; Adria C. Updike ; Hendrik van Eerten ; Karla Varela ;
Date 10 Sep 2015
AbstractA new class of ultra-long duration (>10,000 s) gamma-ray bursts has recently been suggested. They may originate in the explosion of stars with much larger radii than normal long gamma-ray bursts or in the tidal disruptions of a star. No clear supernova had yet been associated with an ultra-long gamma-ray burst. Here we report that a supernova (2011kl) was associated with the ultra-long duration burst 111209A, at z=0.677. This supernova is more than 3 times more luminous than type Ic supernovae associated with long gamma-ray bursts, and its spectrum is distinctly different. The continuum slope resembles those of super-luminous supernovae, but extends farther down into the rest-frame ultra-violet implying a low metal content. The light curve evolves much more rapidly than super-luminous supernovae. The combination of high luminosity and low metal-line opacity cannot be reconciled with typical type Ic supernovae, but can be reproduced by a model where extra energy is injected by a strongly magnetized neutron star (a magnetar), which has also been proposed as the explanation for super-luminous supernovae.
Source arXiv, 1509.3279
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