Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31823
Titolo: | The supernova of the MAGIC GRB190114C | Autori: | MELANDRI, Andrea Izzo, L. PIAN, Elena Malesani, D. B. DELLA VALLE, Massimo ROSSI, Andrea D'Avanzo, P. Guetta, D. Mazzali, P. A. BENETTI, Stefano MASETTI, NICOLA PALAZZI, ELIANA Savaglio, S. AMATI, LORENZO ANTONELLI, Lucio Angelo Ashall, C. BERNARDINI, Maria Grazia CAMPANA, Sergio CARINI, Roberta COVINO, Stefano D'Elia, V. de Ugarte Postigo, A. De Pasquale, M. Filippenko, A. V. Fruchter, A. S. Fynbo, J. P. U. Giunta, A. Hartmann, D. H. Jakobsson, P. Japelj, J. Jonker, P. G. Kann, D. A. Lamb, G. P. Levan, A. J. Martin-Carrillo, A. Moller, P. PIRANOMONTE, Silvia Pugliese, G. SALVATERRA, Ruben Schulze, S. Starling, R. L. C. STELLA, Luigi TAGLIAFERRI, Gianpiero Tanvir, N. Watson, D. |
Data pubblicazione: | 2022 | Rivista: | ASTRONOMY & ASTROPHYSICS | Numero: | 659 | Da pagina:: | A39 | Abstract: | We observed GRB190114C (redshift z = 0.4245), the first GRB ever detected at TeV energies, at optical and near-infrared wavelengths with several ground-based telescopes and the Hubble Space Telescope, with the primary goal of studying its underlying supernova, SN2019jrj. The monitoring spanned the time interval between 1.3 and 370 days after the burst, in the observer frame. We find that the afterglow emission can be modelled with a forward shock propagating in a uniform medium modified by time-variable extinction along the line of sight. A jet break could be present after 7 rest-frame days, and accordingly the maximum luminosity of the underlying SN ranges between that of stripped-envelope corecollapse supernovae (SNe) of intermediate luminosity, and that of the luminous GRB-associated SN2013dx. The observed spectral absorption lines of SN2019jrj are not as broad as in classical GRB-SNe, and are rather more similar to those of less-luminous core-collapse SNe. Taking the broad-lined stripped-envelope core-collapse SN2004aw as an analogue, we tentatively derive the basic physical properties of SN2019jrj. We discuss the possibility that a fraction of the TeV emission of this source might have had a hadronic origin and estimate the expected high-energy neutrino detection level with IceCube. | URI: | http://hdl.handle.net/20.500.12386/31823 | URL: | https://www.aanda.org/articles/aa/abs/2022/03/aa41788-21/aa41788-21.html http://arxiv.org/abs/2112.04759v1 |
ISSN: | 0004-6361 | DOI: | 10.1051/0004-6361/202141788 | Fulltext: | open |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
Melandri_2021_GRB190114C_2112.04759.pdf | preprint | 762.44 kB | Adobe PDF | Visualizza/apri |
aa41788-21.pdf | Pdf editoriale | 700.82 kB | Adobe PDF | Visualizza/apri |
Page view(s)
70
controllato il 11-set-2024
Download(s)
31
controllato il 11-set-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.