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SN 2015bh: NGC 2770's 4th supernova or a luminous blue variable on its way to a Wolf-Rayet star?
C. C. Thöne, A. de Ugarte Postigo, G. Leloudas +13
Very massive stars in the final phases of their lives often show unpredictable outbursts that can mimic supernovae, so-called, "SN impostors", but the distinction is not always str…
The Observer's Guide to the Gamma-Ray Burst-Supernova Connection
Zach Cano, Shan-Qin Wang, Zi-Gao Dai +1
In this review we present a progress report of the connection between long-duration gamma-ray bursts (GRBs) and their accompanying supernovae (SNe). The analysis is from the point…
The 80 Ms follow-up of the X-ray afterglow of GRB 130427A challenges the standard forward shock model
M. De Pasquale, M. J. Page, D. A. Kann +12
GRB 130427A was the brightest gamma-ray burst detected in the last 30 years. With an equivalent isotropic energy output of erg and redshift , it uniquely…
A self-consistent analytical magnetar model: The luminosity of -ray burst supernovae is powered by radioactivity
Zach Cano, Andreas K. G. Johansson, Keiichi Maeda
We present an analytical model that considers energy arising from a magnetar central engine. The results of fitting this model to the optical and X-ray light curves (LCs) of five l…