The environment of the SN-less GRB 111005A at z = 0.0133

The collapsar model has proved highly successful in explaining the properties of long γ-ray bursts (GRBs), with the most direct confirmation being the detection of a supernova (SN) coincident with the majority of nearby long GRBs. Within this model, a long GRB is produced by the core-collapse of a m...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2018-07, Vol.615, p.A136
Hauptverfasser:	Tanga, M., Krühler, T., Schady, P., Klose, S., Graham, J. F., Greiner, J., Kann, D. A., Nardini, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Environmental conditions Galaxies galaxies: abundances galaxies: ISM galaxies: star formation Gamma ray bursts Gamma rays gamma-ray burst: general gamma-ray burst: individual: GRB 111005A Massive stars Metallicity Metals Spectral analysis Star & galaxy formation Star formation Stellar rotation
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