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Related papers: The Observer's Guide to the Gamma-Ray Burst-Supern…

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In this paper we present a correlation between the peak spectral energy of gamma-ray bursts (GRBs) and the peak bolometric luminosity of the underlying supernovae (SNe), based on a sample of four pairs of GRBs-SNe with spectroscopically…

Astrophysics · Physics 2008-11-26 Li-Xin Li

A rapidly spinning, millisecond magnetar is widely considered one of the most plausible power sources for gamma-ray burst-associated supernovae (GRB-SNe). Recent studies have demonstrated that the magnetar model can effectively explain the…

High Energy Astrophysical Phenomena · Physics 2024-11-21 Amit Kumar , Kaushal Sharma

We review the observational status of the Supernova (SN)/Gamma-Ray Burst (GRB) connection. In section 2 we provide a short summary of the observational properties of core-collapse SNe. In sections 3-6 we review the circumstantial evidences…

Astrophysics · Physics 2010-11-11 M. Della Valle

Context: Observations suggest that the major fraction of long duration gamma-ray bursts (GRBs) are connected with broad-lines supernovae Ib/c, (SNe-Ibc). The presence of GRB-SNe is revealed by rebrightenings emerging from the optical GRB…

High Energy Astrophysical Phenomena · Physics 2014-10-01 M. Kovacevic , L. Izzo , Y. Wang , M. Muccino , M. Della Valle , L. Amati , C. Barbarino , M. Enderli , G. B. Pisani , L. Li

Gamma-Ray Bursts (GRBs) are very energetic cosmological transients. Long GRBs are usually associated with Type Ib/c Supernovae (SNe), and we refer to them as GRB-SNe. Since the associated SN for a given GRB is observed only at low redshift,…

High Energy Astrophysical Phenomena · Physics 2022-10-13 M. G. Dainotti , B. De Simone , M. I. Khadir , K. Kawaguchi , T. J. Moriya , T. Takiwaki , N. Tominaga , A. Gangopadhyay

We systematically compare the temporal and spectral properties of 53 Supernova (SN)-associated and 15 Kilonova (KN)-associated Gamma-Ray Bursts (GRBs). We find that the spectral parameters of both types GRBs are identically and lognormally…

High Energy Astrophysical Phenomena · Physics 2023-09-19 Q. M. Li , Z. B. Zhang , X. L. Han , K. J. Zhang , X. L. Xia , C. T. Hao

Observations show that at least some gamma-ray bursts (GRBs) happen simultaneously with core-collapse supernovae (SNe), thus linking by a common thread nature's two grandest explosions. We review here the growing evidence for and…

Astrophysics · Physics 2008-11-26 S. E. Woosley , J. S. Bloom

Long-duration gamma-ray bursts (GRBs) are believed to be produced by the core collapse of massive stars and hence to be connected with supernovae (SNe). Indeed, for four pairs of GRBs and SNe, spectroscopically confirmed connection has been…

Astrophysics · Physics 2009-11-13 Li-Xin Li

Unique data on $BVRI$ light curves of the optical transient (OT) of GRB 970508 obtained with the 6-m telescope have been interpreted in the framework of the idea of a straightforward link between supernovae (SNe) and long duration gamma-ray…

Astrophysics · Physics 2007-05-23 V. V. Sokolov

We present optical and near-infrared photometry of GRB~140606B ($z=0.384$), and optical photometry and spectroscopy of its associated supernova (SN). The results of our modelling indicate that the bolometric properties of the SN ($M_{\rm…

The favored progenitor model for Gamma-ray Bursts (GRBs) with Supernova (SN) association is the core collapse of massive stars. One possible outcome of such a collapse is a rapidly spinning, strongly magnetized neutron star ("magnetar"). We…

High Energy Astrophysical Phenomena · Physics 2018-08-08 Hou-Jun Lü , Lin Lan , Bing Zhang , En-Wei Liang , David Alexander Kann , Shen-Shi Du , Jun Shen

Over the last few years our understanding of local Type Ibc supernovae and their connection to long-duration gamma-ray bursts has been revolutionized. Recent discoveries have shown that the emerging picture for core-collapse explosions is…

Astrophysics · Physics 2009-11-11 A. M. Soderberg

The connection between long GRBs and supernovae is now well established. I briefly review the evidence in favor of this connection and summarise where we are observationally. I also use a few events to exemplify what should be done and what…

High Energy Astrophysical Phenomena · Physics 2012-07-02 David Bersier

We review the observational status of the supernova/gamma-ray burst connection. Present data suggest that SNe associated with GRBs form a heterogeneous class of objects including both bright and faint hypernovae and perhaps also `standard'…

Astrophysics · Physics 2009-11-11 Massimo Della Valle

Gamma Ray Bursts (GRBs) and Supernovae (SNe) are among the brightest and most energetic physical processes in the universe. It is known that core-collapse SNe arise from the gravitational collapse and subsequent explosion of massive stars…

High Energy Astrophysical Phenomena · Physics 2012-08-02 Zach Cano

Multiple observational lines of evidence support a connection between hydrogen-poor superluminous supernovae (SLSNe) and long duration gamma-ray bursts (GRBs). Both events require a powerful central energy source, usually attributed to a…

High Energy Astrophysical Phenomena · Physics 2018-01-24 Ben Margalit , Brian D. Metzger , Todd A. Thompson , Matt Nicholl , Tuguldur Sukhbold

Observations of several gamma-ray bursts (GRBs) that are temporally and spatially compatible with energetic supernovae (hypernovae) has established their common origin. In one case (GRB 111209A/SN 2011kl) the associated supernova was…

High Energy Astrophysical Phenomena · Physics 2025-05-08 Achille Fiore , Ludovica Crosato Menegazzi , Giulia Stratta

Long-duration gamma-ray bursts (GRBs) have been often considered as the natural evolution of some core-collapse supernovae (SNe). While GRBs with relativistic jets emit an electromagnetic signal, GRBs with mildly relativistic jets are…

High Energy Astrophysical Phenomena · Physics 2016-03-23 Irene Tamborra , Shin'ichiro Ando

The association between long gamma-ray bursts (LGRBs) and core-collapse supernovae (SNe) has been well established since the discovery of SN 1998bw, which was linked to the low-luminosity LGRB 980425. However, long-term monitoring of…

High Energy Astrophysical Phenomena · Physics 2025-10-24 Xiao-Fei Dong , Yong-Feng Huang , Zhi-Bin Zhang , Jin-Jun Geng , Chen Deng , Ze-Cheng Zou , Chen-Ran Hu , Orkash Amat
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