Highly luminous supernovae associated with gamma-ray bursts I. GRB 111209A/SN 2011kl in the context of stripped-envelope and superluminous supernovae
- NázevTitle
- Highly luminous supernovae associated with gamma-ray bursts I. GRB 111209A/SN 2011kl in the context of stripped-envelope and superluminous supernovaeHighly luminous supernovae associated with gamma-ray bursts I. GRB 111209A/SN 2011kl in the context of stripped-envelope and superluminous supernovae
- Druh výsledkuResult type
- Článek v časopiseJournal article
- AutořiAuthors
- D. A. Kann, P. Schady, F. E. Olivares, S. Klose, R. Filgas
- DOIDOI
- 10.1051/0004-6361/201629162
- Časopis / citaceJournal / citation
- Astronomy & Astrophysics. 2019, 624 143-161. ISSN 1432-0746.
- RokYear
- 2019
- JazykLanguage
- eng
- WoSWoS
- 000465638000006
- ScopusScopus
- 2-s2.0-85065233422
- RIVRIV
- RIV/68407700:21670/19:00335742!RIV20-MSM-21670___
- ProjektProject
- Inženýrské aplikace fyziky mikrosvětaEngineering applications of microworld physics
AbstraktAbstract
Context. GRB 111209A, one of the longest gamma-ray bursts (GRBs) ever observed, is linked to SN 2011kl, which is the most luminous GRB supernova (SN) detected so far. Several lines of evidence indicate that this GRB-SN is powered by a magnetar central engine.
Context. GRB 111209A, one of the longest gamma-ray bursts (GRBs) ever observed, is linked to SN 2011kl, which is the most luminous GRB supernova (SN) detected so far. Several lines of evidence indicate that this GRB-SN is powered by a magnetar central engine.