GRB 190114C in the nuclear region of an interacting galaxy A detailed host analysis using ALMA, the HST, and the VLT

de Ugarte Postigo, A.; Thone, C.; Martin, S.; Japelj, J.; Levan, A.; Michalowski, M.; Selsing, J.; Kann, D.; Schulze, S.; Palmerio, J.; Vergani, S.; Tanvir, N.; Bensch, K.; Covino, S.; D'Elia, V; De Pasquale, M.; Fruchter, A.; Fynbo, J.; Hartmann, D.; Heintz, K.; van der Horst, A.; Izzo, L.; Jakobsson, P.; Ng, K.; Perley, D.; Rossi, A.; Sbarufatti, B.; Salvaterra, R.; Sanchez-Ramirez, R.; Watson, D.; Xu, D.

doi:10.1051/0004-6361/201936668

GRB 190114C in the nuclear region of an interacting galaxy A detailed host analysis using ALMA, the HST, and the VLT

de Ugarte Postigo A., Thone C. C., Martin S., Japelj J., Levan A. J., Michalowski M. J., ...Daha Fazla

ASTRONOMY & ASTROPHYSICS, cilt.633, 2020 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 633
Basım Tarihi: 2020
Doi Numarası: 10.1051/0004-6361/201936668
Dergi Adı: ASTRONOMY & ASTROPHYSICS
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus, Academic Search Premier, Aerospace Database, Artic & Antarctic Regions, Communication Abstracts, Compendex, INSPEC, Metadex, zbMATH, DIALNET, Civil Engineering Abstracts
İstanbul Üniversitesi Adresli: Evet

Özet

Context. For the first time, very high energy emission up to the TeV range has been reported for a gamma-ray burst (GRB). It is still unclear whether the environmental properties of GRB 190114C might have contributed to the production of these very high energy photons, or if it is solely related to the released GRB emission.