The supernova of the MAGIC gamma-ray burst GRB190114C

被引：16

作者：

Melandri, A. ^{[1
]}

Izzo, L. ^{[2
]}

Pian, E. ^{[3
,4
]}

Malesani, D. B. ^{[2
,5
,6
,7
]}

Della Valle, M. ^{[8
,9
,10
]}

Rossi, A. ^{[3
]}

D'Avanzo, P. ^{[1
]}

Guetta, D. ^{[11
,12
]}

Mazzali, P. A. ^{[4
,13
]}

Benetti, S. ^{[14
]}

Masetti, N. ^{[3
,15
]}

Palazzi, E. ^{[3
]}

Savaglio, S. ^{[16
]}

Amati, L. ^{[3
]}

Antonelli, L. A. ^{[17
]}

Ashall, C. ^{[18
]}

Bernardini, M. G. ^{[1
]}

Campana, S. ^{[1
]}

Carini, R. ^{[17
]}

Covino, S. ^{[1
]}

D'Elia, V ^{[17
,19
]}

de Ugarte Postigo, A. ^{[20
]}

De Pasquale, M. ^{[21
]}

Filippenko, A., V ^{[22
,23
]}

Fruchter, A. S. ^{[24
]}

Fynbo, J. P. U. ^{[6
,7
]}

Giunta, A. ^{[19
]}

Hartmann, D. H. ^{[25
]}

Jakobsson, P. ^{[26
]}

Japelj, J. ^{[27
]}

Jonker, P. G. ^{[28
,29
]}

Kann, D. A. ^{[20
]}

Lamb, G. P. ^{[30
]}

Levan, A. J. ^{[28
]}

Martin-Carrillo, A. ^{[31
]}

Moller, P. ^{[32
]}

Piranomonte, S. ^{[17
]}

Pugliese, G. ^{[27
]}

Salvaterra, R. ^{[33
]}

Schulze, S. ^{[34
]}

Starling, R. L. C. ^{[30
]}

Stella, L. ^{[17
]}

Tagliaferri, G. ^{[1
]}

Tanvir, N. ^{[30
]}

Watson, D. ^{[6
,7
]}

机构：

[1] INAF Osservatorio Astron Brera, Via E Bianchi 46, I-23807 Merate, LC, Italy

[2] Univ Copenhagen, Niels Bohr Inst, DARK, Jagtvej 128, DK-2200 Copenhagen N, Denmark

[3] INAF Osservatorio Astrofis & Sci Spazio, Via P Gobetti 101, I-40129 Bologna, Italy

[4] Liverpool JMU, Astrophys Res Inst, IC2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England

[5] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark

[6] Cosm Dawn Ctr Dawn, Copenhagen, Denmark

[7] Univ Copenhagen, Niels Bohr Inst, Jagtvej 128, DK-2200 Copenhagen N, Denmark

[8] INAF Osservatorio Astron Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy

[9] INFN Napoli, Str Comunale Cinthia, I-80126 Naples, NA, Italy

[10] ICRANet, Piazza Repubbl 10, I-65122 Pescara, Italy

[11] Univ Ariel, Phys Dept, Ariel, West Bank, Israel

[12] ORT Braude Coll, Dept Phys, Snunit St 51, IL-2161002 Karmiel, Israel

[13] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany

[14] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy

[15] Univ Andres Bello, Dept Ciencias Fis, Fernandez Concha 700, Santiago, Chile

[16] Univ Calabria, Phys Dept, I-87036 Arcavacata Di Rende, Cs, Italy

[17] INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, RM, Italy

[18] Univ Hawaii Manoa, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA

[19] Agenzia Spaziale Italiana ASI, Space Sci Data Ctr SSDC, Via Politecn, I-00133 Rome, Italy

[20] Inst Astrofis Andalucia IAA CSIC, Glorieta Astron S-N, Granada 18008, Spain

[21] Istanbul Univ, Dept Astron & Space Sci, TR-34119 Istanbul, Turkey

[22] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[23] Univ Calif Berkeley, Miller Inst Basic Res Sci, Berkeley, CA 94720 USA

[24] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[25] Clemson Univ, Dept Phys & Astron, Clemson, SC 29634 USA

[26] Univ Iceland, Sci Inst, Ctr Astrophys & Cosmol, Dunhagi 5, IS-107 Reykjavik, Iceland

[27] Univ Amsterdam, Anton Pannekoek Inst Astron, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[28] Radboud Univ Nijmegen, Dept Astrophys, NL-6525 AJ Nijmegen, Netherlands

[29] SRON Netherlands Inst Space Res, SRON, Sorbonnelaan 2, NL-3584 CA Utrecht, Netherlands

[30] Univ Leicester, Sch Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, England

[31] Univ Coll Dublin, Sch Phys, Dublin 4, Ireland

[32] ESO Headquarters, Karl Schwarzschildstr 2, D-85748 Garching, Germany

[33] INAF Ist Astrofis Spaziale & Fis Cosm, Via A Corti 12, I-20133 Milan, Italy

[34] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot, Israel

来源：

ASTRONOMY & ASTROPHYSICS | 2022年 / 659卷

基金：

新加坡国家研究基金会;

关键词：

gamma-ray burst: individual: GRB 190114C; supernovae: individual: SN 2019jrj; LIGHT; FERMI; TELESCOPE; SPECTRUM; STAR; JET;

D O I：

10.1051/0004-6361/202141788

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We observed GRB 190114C (redshift z = 0.4245), the first gamma-ray burst (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, SN 2019jrj. 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 supernova (SN) ranges between that of stripped-envelope core-collapse SNe of intermediate luminosity and that of the luminous GRB-associated SN 2013dx. The observed spectral absorption lines of SN 2019jrj are not as broad as in classical GRB SNe and are instead more similar to those of less-luminous core-collapse SNe. Taking the broad-lined stripped-envelope core-collapse SN 2004aw as an analogue, we tentatively derive the basic physical properties of SN 2019jrj. 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.

引用

页数：9

共 50 条

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