Issue |
A&A
Volume 686, June 2024
|
|
---|---|---|
Article Number | A149 | |
Number of page(s) | 17 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/202348374 | |
Published online | 07 June 2024 |
Unveiling extended gamma-ray emission around HESS J1813-178
1
Dublin Institute for Advanced Studies,
31 Fitzwilliam Place,
Dublin 2,
Ireland
2
Max-Planck-Institut für Kernphysik,
PO Box 103980,
D 69029
Heidelberg,
Germany
3
Yerevan Physics Institute,
2 Alikhanian Brothers St.,
Yerevan
0036,
Armenia
4
Yerevan State University,
1 Alek Manukyan St,
Yerevan
0025,
Armenia
5
Landessternwarte, Universität Heidelberg,
Königstuhl,
69117
Heidelberg,
Germany
6
Kapteyn Astronomical Institute, University of Groningen,
Landleven 12,
9747 AD
Groningen,
The Netherlands
7
Laboratoire Leprince-Ringuet, École Polytechnique, CNRS, Institut Polytechnique de Paris,
91128
Palaiseau,
France
8
University of Namibia, Department of Physics,
Private Bag 13301,
Windhoek
10005,
Namibia
9
Centre for Space Research, North-West University,
Potchefstroom
2520,
South Africa
10
Universität Hamburg, Institut für Experimentalphysik,
Luruper Chaussee 149,
22761
Hamburg,
Germany
11
Deutsches Elektronen-Synchrotron DESY,
Platanenallee 6,
15738
Zeuthen,
Germany
12
Department of Physics, University of the Free State,
PO Box 339,
Bloemfontein
9300,
South Africa
13
Institut für Physik und Astronomie, Universität Potsdam,
Karl-Liebknecht-Strasse 24/25,
14476
Potsdam,
Germany
14
Université Paris Cité, CNRS,
Astroparticule et Cosmologie,
75013
Paris,
France
15
Department of Physics and Electrical Engineering, Linnaeus University,
351 95
Växjö,
Sweden
16
Institut für Physik, Humboldt-Universität zu Berlin,
Newtonstr. 15,
12489
Berlin,
Germany
17
Institut für Astronomie und Astrophysik, Universität Tübingen,
Sand 1,
72076
Tübingen,
Germany
18
Laboratoire Univers et Théories, Observatoire de Paris, Université PSL, CNRS, Université Paris Cité,
5 Pl. Jules Janssen,
92190
Meudon,
France
19
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
20
IRFU, CEA, Université Paris-Saclay,
91191
Gif-sur-Yvette,
France
21
Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics,
Nikolaus-Fiebiger-Str. 2,
91058
Erlangen,
Germany
22
Astronomical Observatory, The University of Warsaw,
Al. Ujazdowskie 4,
00-478
Warsaw,
Poland
23
Université Savoie Mont Blanc, CNRS, Laboratoire d’Annecy de Physique des Particules - IN2P3,
74000
Annecy,
France
24
Instytut Fizyki Ja̧drowej PAN,
ul. Radzikowskiego 152,
31-342
Kraków,
Poland
25
Université Bordeaux, CNRS,
LP2I Bordeaux, UMR 5797,
33170
Gradignan,
France
26
School of Physics, University of the Witwatersrand,
1 Jan Smuts Avenue, Braamfontein,
Johannesburg,
2050
South Africa
27
University of Oxford, Department of Physics,
Denys Wilkinson Building, Keble Road,
Oxford
OX1 3RH,
UK
28
School of Physical Sciences, University of Adelaide,
Adelaide
5005,
Australia
29
Aix Marseille Université, CNRS/IN2P3, CPPM,
Marseille,
France
30
Laboratoire Univers et Particules de Montpellier, Université Montpellier, CNRS/IN2P3,
CC 72, Place Eugène Bataillon,
34095
Montpellier Cedex 5,
France
31
Universität Innsbruck, Institut für Astro- und Teilchenphysik,
Technikerstraße 25,
6020
Innsbruck,
Austria
32
Obserwatorium Astronomiczne, Uniwersytet Jagielloński,
ul. Orla 171,
30-244
Kraków,
Poland
33
Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University,
Grudziadzka 5,
87-100
Torun,
Poland
34
Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences,
ul. Bartycka 18,
00-716
Warsaw,
Poland
35
Department of Physics and Astronomy, The University of Leicester,
University Road,
Leicester,
LE1 7RH,
UK
36
GRAPPA, Anton Pannekoek Institute for Astronomy, University of Amsterdam,
Science Park 904,
1098 XH
Amsterdam,
The Netherlands
37
Department of Physics, Konan University,
8-9-1 Okamoto, Higashinada, Kobe,
Hyogo
658-8501,
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,
Chiba,
277-8583,
Japan
39
RIKEN,
2-1 Hirosawa, Wako,
Saitama
351-0198,
Japan
40
School of Science, Western Sydney University,
Locked Bag 1797,
Penrith South DC,
NSW 2751,
Australia
Received:
24
October
2023
Accepted:
21
March
2024
Context. HESS J1813–178 is a very-high-energy γ-ray source spatially coincident with the young and energetic pulsar PSR J1813–1749 and thought to be associated with its pulsar wind nebula (PWN). Recently, evidence for extended high-energy emission in the vicinity of the pulsar has been revealed in the Fermi Large Area Telescope (LAT) data. This motivates revisiting the HESS J1813–178 region, taking advantage of improved analysis methods and an extended dataset.
Aims. Using data taken by the High Energy Stereoscopic System (H.E.S.S.) experiment and the Fermi-LAT, we aim to describe the γ-ray emission in the region with a consistent model, to provide insights into its origin.
Methods. We performed a likelihood-based analysis on 32 hours of H.E.S.S. data and 12 yr of Fermi-LAT data and we fitted a spectro-morphological model to the combined datasets. These results allowed us to develop a physical model for the origin of the observed γ-ray emission in the region.
Results. In addition to the compact very-high-energy γ-ray emission centred on the pulsar, we find a significant yet previously undetected component along the Galactic plane. With Fermi-LAT data, we confirm extended high-energy emission consistent with the position and elongation of the extended emission observed with H.E.S.S. These results establish a consistent description of the emission in the region from GeV energies to several tens of TeV.
Conclusions. This study suggests that HESS J1813–178 is associated with a γ-ray PWN powered by PSR J1813–1749. A possible origin of the extended emission component is inverse Compton emission from electrons and positrons that have escaped the confines of the pulsar and form a halo around the PWN.
Key words: pulsars: individual: PSR J1813-1749 / gamma rays: general / gamma rays: ISM
© The Authors 2024
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.
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