Issue |
A&A
Volume 626, June 2019
|
|
---|---|---|
Article Number | A57 | |
Number of page(s) | 11 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201935242 | |
Published online | 12 June 2019 |
Upper limits on very-high-energy gamma-ray emission from core-collapse supernovae observed with H.E.S.S.
1
Centre for Space Research, North-West University,
Potchefstroom
2520,
South Africa
2
Universität Hamburg, Institut für Experimentalphysik,
Luruper Chaussee 149,
22761
Hamburg,
Germany
3
Max-Planck-Institut für Kernphysik,
PO Box 103980,
69029
Heidelberg,
Germany
4
Dublin Institute for Advanced Studies,
31 Fitzwilliam Place,
Dublin 2,
Ireland
5
High Energy Astrophysics Laboratory, RAU,
123 Hovsep Emin St
Yerevan
0051,
Armenia
6
Yerevan Physics Institute,
2 Alikhanian Brothers St.,
375036
Yerevan,
Armenia
7
Institut für Physik, Humboldt-Universität zu Berlin,
Newtonstr. 15,
12489
Berlin,
Germany
8
Department of Physics, University of Namibia,
Private Bag 13301,
Windhoek,
12010,
Namibia
9
GRAPPA, Anton Pannekoek Institute for Astronomy, University of Amsterdam,
Science Park 904,
1098 XH
Amsterdam,
The Netherlands
10
Department of Physics and Electrical Engineering, Linnaeus University,
351 95
Växjö,
Sweden
11
Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und Astrophysik, Ruhr-Universität Bochum,
44780
Bochum,
Germany
12
Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität Innsbruck,
6020
Innsbruck,
Austria
13
School of Physical Sciences, University of Adelaide,
Adelaide
5005,
Australia
14
LUTH, Observatoire de Paris, PSL Research University, CNRS, Université Paris Diderot,
5 Place Jules Janssen,
92190
Meudon,
France
15
Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies, LPNHE,
4 Place Jussieu,
75252
Paris,
France
16
Laboratoire Univers et Particules de Montpellier, Université Montpellier, CNRS/IN2P3, CC 72,
Place Eugène Bataillon,
34095
Montpellier Cedex 5,
France
17
IRFU, CEA, Université Paris-Saclay,
91191
Gif-sur-Yvette,
France
18
Astronomical Observatory, The University of Warsaw,
Al. Ujazdowskie 4,
00-478
Warsaw,
Poland
19
Aix Marseille Université, CNRS/IN2P3, CPPM,
Marseille,
France
20
Instytut Fizyki Ja̧drowej PAN,
ul. Radzikowskiego 152,
31-342
Kraków,
Poland
21
School of Physics, University of the Witwatersrand,
1 Jan Smuts Avenue,
Braamfontein,
Johannesburg
2050,
South Africa
22
Laboratoire d’Annecy de Physique des Particules, Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS, LAPP,
74000
Annecy,
France
23
Landessternwarte, Universität Heidelberg,
Königstuhl,
69117
Heidelberg,
Germany
24
Université Bordeaux, CNRS/IN2P3, Centre d’Études Nucléaires de Bordeaux Gradignan,
33175
Gradignan,
France
25
Institut für Astronomie und Astrophysik, Universität Tübingen,
Sand 1,
72076
Tübingen,
Germany
26
Laboratoire Leprince-Ringuet, École Polytechnique, UMR 7638, CNRS/IN2P3, Institut Polytechnique de Paris,
91128
Palaiseau,
France
27
APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris,
Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet,
75205
Paris Cedex 13,
France
28
Université Grenoble Alpes, CNRS, IPAG,
38000
Grenoble,
France
29
Department of Physics and Astronomy, The University of Leicester University Road,
Leicester,
LE1 7RH,
UK
30
Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences,
ul. Bartycka 18,
00-716
Warsaw,
Poland
31
Institut für Physik und Astronomie, Universität Potsdam,
Karl-Liebknecht-Strasse 24/25,
14476
Potsdam,
Germany
32
Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics,
Erwin-Rommel-Str. 1,
91058
Erlangen,
Germany
33
DESY,
15738
Zeuthen,
Germany
34
Obserwatorium Astronomiczne, Uniwersytet Jagielloński,
ul. Orla 171,
30-244
Kraków,
Poland
35
Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University,
Grudziadzka 5,
87-100
Torun,
Poland
36
Department of Physics, University of the Free State,
PO Box 339,
Bloemfontein
9300,
South Africa
37
Department of Physics, Rikkyo University,
3-34-1 Nishi-Ikebukuro,
Toshima-ku,
Tokyo
171-8501,
Japan
38
Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study (UTIAS), The University of Tokyo,
5-1-5 Kashiwa-no-Ha,
Kashiwa City,
Chiba
277-8583,
Japan
39
Department of Physics, The University of Tokyo,
7-3-1 Hongo,
Bunkyo-ku,
Tokyo
113-0033,
Japan
40
RIKEN,
2-1 Hirosawa,
Wako,
Saitama
351-0198,
Japan
41
Now at Physik Institut, Universität Zürich,
Winterthurerstrasse 190,
8057
Zürich,
Switzerland
42
Now at Institut de Ciències del Cosmos (ICC UB), Universitat de Barcelona (IEEC-UB),
Martí Franquès 1,
08028
Barcelona,
Spain
43
School of Sciences, University of New South Wales, Australian Defence Force Academy,
Canberra,
ACT
2600,
Australia
Received:
10
February
2019
Accepted:
15
April
2019
Young core-collapse supernovae with dense-wind progenitors may be able to accelerate cosmic-ray hadrons beyond the knee of the cosmic-ray spectrum, and this may result in measurable gamma-ray emission. We searched for gamma-ray emission from ten supernovae observed with the High Energy Stereoscopic System (H.E.S.S.) within a year of the supernova event. Nine supernovae were observed serendipitously in the H.E.S.S. data collected between December 2003 and December 2014, with exposure times ranging from 1.4 to 53 h. In addition we observed SN 2016adj as a target of opportunity in February 2016 for 13 h. No significant gamma-ray emission has been detected for any of the objects, and upper limits on the >1 TeV gamma-ray flux of the order of ~10−13 cm−2s−1 are established, corresponding to upper limits on the luminosities in the range ~2 × 1039 to ~1 × 1042 erg s−1. These values are used to place model-dependent constraints on the mass-loss rates of the progenitor stars, implying upper limits between ~2 × 10−5 and ~2 × 10−3 M⊙ yr−1 under reasonable assumptions on the particle acceleration parameters.
Key words: gamma rays: general / supernovae: general / cosmic rays
© ESO 2019
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