Issue |
A&A
Volume 644, December 2020
|
|
---|---|---|
Article Number | A112 | |
Number of page(s) | 8 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/202038851 | |
Published online | 07 December 2020 |
An extreme particle accelerator in the Galactic plane: HESS J1826−130
1
Centre for Space Research, North-West University,
Potchefstroom
2520, South Africa
2
Laboratoire Leprince-Ringuet, école Polytechnique, CNRS, Institut Polytechnique de Paris,
91128
Palaiseau, France
3
Dublin Institute for Advanced Studies,
31 Fitzwilliam Place,
Dublin 2,
Ireland
4
Max-Planck-Institut für Kernphysik,
PO Box 103980,
69029
Heidelberg,
Germany
5
High Energy Astrophysics Laboratory, RAU,
123 Hovsep Emin
St Yerevan
0051, Armenia
6
Aix-Marseille Université, CNRS/IN2P3, CPPM,
Marseille, France
7
Laboratoire d’Annecy de Physique des Particules, Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, LAPP,
74000
Annecy,
France
8
University of Oxford, Department of Physics,
Denys Wilkinson Building, Keble Road,
Oxford
OX1 3RH, UK
9
IRFU, CEA, Université Paris-Saclay,
91191
Gif-sur-Yvette, France
10
University of Namibia, Department of Physics,
Private Bag 13301,
Windhoek
10005,
Namibia
11
Instytut Fizyki Ja̧drowej PAN,
ul. Radzikowskiego 152,
31-342
Kraków,
Poland
12
DESY,
15738
Zeuthen,
Germany
13
Obserwatorium Astronomiczne, Uniwersytet Jagielloński,
ul. Orla 171,
30-244
Kraków, Poland
14
Department of Physics and Electrical Engineering, Linnaeus University,
351 95
Växjö,
Sweden
15
Institut für Astronomie und Astrophysik, Universität Tübingen,
Sand 1,
72076
Tübingen, Germany
16
Laboratoire Univers et Théories, Observatoire de Paris, Université PSL, CNRS, Université de Paris,
92190
Meudon,
France
17
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
18
GRAPPA, Anton Pannekoek Institute for Astronomy, University of Amsterdam,
Science Park 904,
1098 XH
Amsterdam, The Netherlands
19
Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics,
Erwin-Rommel-Str. 1,
91058
Erlangen, Germany
20
Astronomical Observatory, The University of Warsaw,
Al. Ujazdowskie 4,
00-478
Warsaw,
Poland
21
School of Physics, University of the Witwatersrand,
1 Jan Smuts Avenue,
Braamfontein,
Johannesburg
2050,
South Africa
22
Université Bordeaux, CNRS/IN2P3, Centre d’Études Nucléaires de Bordeaux Gradignan,
33175
Gradignan, France
23
School of Physical Sciences, University of Adelaide,
Adelaide
5005, Australia
24
Universität Hamburg, Institut für Experimentalphysik,
Luruper Chaussee 149,
22761
Hamburg, Germany
25
Université de Paris, CNRS, Astroparticule et Cosmologie,
75013
Paris, France
26
Department of Physics and Astronomy, The University of Leicester, University Road,
Leicester,
LE1 7RH, UK
27
Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences,
ul. Bartycka 18,
00-716
Warsaw,
Poland
28
Institut für Physik und Astronomie, Universität Potsdam,
Karl-Liebknecht-Strasse 24/25,
14476
Potsdam, Germany
29
Laboratoire Univers et Particules de Montpellier, Université Montpellier,
CNRS/IN2P3, CC 72, Place Eugène Bataillon,
34095
Montpellier Cedex 5, France
30
Landessternwarte, Universität Heidelberg, Königstuhl,
D 69117
Heidelberg, Germany
31
Institut für Physik, Humboldt-Universität zu Berlin,
Newtonstr. 15,
12489
Berlin, Germany
32
Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität Innsbruck,
6020
Innsbruck, Austria
33
Department of Physics, Rikkyo University,
3-34-1 Nishi-Ikebukuro,
Toshima-ku,
Tokyo
171-8501, Japan
34
Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University,
Grudziadzka 5,
87-100
Torun, Poland
35
Department of Physics, University of the Free State,
PO Box 339,
Bloemfontein
9300, South Africa
36
Department of Physics, The University of Tokyo,
7-3-1 Hongo,
Bunkyo-ku,
Tokyo
113-0033, Japan
37
Yerevan Physics Institute,
2 Alikhanian Brothers St.,
375036
Yerevan,
Armenia
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,
Chiba,
277-8583, Japan
39
Now at Physik Institut, Universität Zürich, Winterthurerstrasse 190,
8057
Zürich, Switzerland
40
Now at Institut de Ciències del Cosmos (ICC UB), Universitat de Barcelona (IEEC-UB),
Martí Franquès 1,
08028
Barcelona, Spain
Received:
6
July
2020
Accepted:
27
September
2020
The unidentified very-high-energy (VHE; E > 0.1 TeV) γ-ray source, HESS J1826−130, was discovered with the High Energy Stereoscopic System (HESS) in the Galactic plane. The analysis of 215 h of HESS data has revealed a steady γ-ray flux from HESS J1826−130, which appears extended with a half-width of 0.21° ± 0.02stat° ± 0.05sys°. The source spectrum is best fit with either a power-law function with a spectral index Γ = 1.78 ± 0.10stat ± 0.20sys and an exponential cut-off at 15.2−3.2+5.5 TeV, or a broken power-law with Γ1 = 1.96 ± 0.06stat ± 0.20sys, Γ2 = 3.59 ± 0.69stat ± 0.20sys for energies below and above Ebr = 11.2 ± 2.7 TeV, respectively. The VHE flux from HESS J1826−130 is contaminated by the extended emission of the bright, nearby pulsar wind nebula, HESS J1825−137, particularly at the low end of the energy spectrum. Leptonic scenarios for the origin of HESS J1826−130 VHE emission related to PSR J1826−1256 are confronted by our spectral and morphological analysis. In a hadronic framework, taking into account the properties of dense gas regions surrounding HESS J1826−130, the source spectrum would imply an astrophysical object capable of accelerating the parent particle population up to ≳200 TeV. Our results are also discussed in a multiwavelength context, accounting for both the presence of nearby supernova remnants, molecular clouds, and counterparts detected in radio, X-rays, and TeV energies.
Key words: ISM: supernova remnants / ISM: clouds / gamma rays: general / gamma rays: ISM
© H.E.S.S. Collaboration 2020
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.