TeV Analysis of a Source-rich Region with the HAWC Observatory: Is HESS J1809-193 a Potential Hadronic PeVatron?

Abstract HESS J1809-193 is an unidentified TeV source, first detected by the High Energy Stereoscopic System (H.E.S.S.) collaboration. The emission originates in a source-rich region that includes several supernova remnants (SNRs) and pulsars including SNR G11.1+0.1, SNR G11.0-0.0, and the young radio pulsar PSR J1809-1917. Originally classified as a pulsar wind nebula candidate, recent studies show the peak of the TeV region overlapping with a system of molecular clouds. This resulted in the revision of the original leptonic scenario to look for alternate hadronic scenarios. Marked as a potential PeVatron candidate, this region has been studied extensively by H.E.S.S. due to its emission extending up to several tens of TeV. In this work, we use 2398 days of data from the High Altitude Water Cherenkov (HAWC) observatory to carry out a systematic source search of the HESS J1809-193 region. We were able to resolve emission detected as an extended component (modelled as a symmetric Gaussian with a 1 σ radius of 0.°21) with no clear cutoff at high energies and emitting photons up to 210 TeV. We model the multiwavelength observations for the region around HESS J1809-193 using a time-dependent leptonic model and a lepto-hadronic model. Our model indicates that both scenarios could explain the observed data within the region of HESS J1809-193.

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Journal
The Astrophysical Journal
Published
2024-08-22
DOI
https://doi.org/10.3847/1538-4357/ad59a6
Citations
3
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
1.98

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article

TeV Analysis of a Source-rich Region with the HAWC Observatory: Is HESS J1809-193 a Potential Hadronic PeVatron?

F. Ureña-Mena, Rishi Babu, E. Belmont‐Moreno, A. Lara et al.
3 citations
The Astrophysical Journal
Astrophysics and Cosmic Phenomena
1.98
article

TeV Analysis of a Source-rich Region with the HAWC Observatory: Is HESS J1809-193 a Potential Hadronic PeVatron?

F. Ureña-Mena, Rishi Babu, E. Belmont‐Moreno, A. Lara, K. Tollefson, Enrique Varela, Y. Pérez Araujo, P. Miranda-Romagnoli, E. De la Fuente, I. Herzog, I. J. Watson, Vikas Joshi, K. Malone, S. Casanova, R. Noriega-Papaqui, L. Nellen, M. Breuhaus, J. A. Goodman, O. Tibolla, José Serna-Franco, E. Willox, Y. Son, J. A. Montes, I. Torres, M. Newbold, G. Luis-Raya, J. S. H. Lee, J. A. Morales-Soto, N. Di Lalla, B. L. Dingus, A. J. Smith, P. Hüntemeyer, X. Wang, C. Espinoza, K. S. Caballero‐Mora, R. W. Springer, Chang Dong Rho, F. Garfias, D. Rosa‐González, A. L. Longinotti, F. Hueyotl‐Zahuantitla, A. Iriarte, M. A. DuVernois, Alfonso Muñoz, A. Sandoval, D. Avila Rojas, A. Albert, Magda Gonzalez, J. P. Harding, E. Ruiz-Velasco, R. Alfaro, M. Mostafá, J. A. García-González, E. G. Pérez-Pérez, J. Martínez-Castro, Kwok Lung Fan, Rhiannon M. Turner, S. Hernández-Cadena, Davide Depaoli, S. Yun-Cárcamo, Marcela Andrea Osorio Osorio, J. A. Matthews, J. Cotzomi, R. Diaz Hernandez, M. U. Nisa, H. León Vargas, D. Huang, Humberto Antonio Salazar Ibarguen, Brian Fick, J. C. Arteaga‐Velázquez, R. Torres-Escobedo, C. Álvarez, E. Moreno, M. Schneider, T. Capistrán, S. Groetsch, S. Kaufmann, N. Fraija, H. Zhou, A. Carramiñana, A. Bernal
article en
3 citations

Abstract

Abstract HESS J1809-193 is an unidentified TeV source, first detected by the High Energy Stereoscopic System (H.E.S.S.) collaboration. The emission originates in a source-rich region that includes several supernova remnants (SNRs) and pulsars including SNR G11.1+0.1, SNR G11.0-0.0, and the young radio pulsar PSR J1809-1917. Originally classified as a pulsar wind nebula candidate, recent studies show the peak of the TeV region overlapping with a system of molecular clouds. This resulted in the revision of the original leptonic scenario to look for alternate hadronic scenarios. Marked as a potential PeVatron candidate, this region has been studied extensively by H.E.S.S. due to its emission extending up to several tens of TeV. In this work, we use 2398 days of data from the High Altitude Water Cherenkov (HAWC) observatory to carry out a systematic source search of the HESS J1809-193 region. We were able to resolve emission detected as an extended component (modelled as a symmetric Gaussian with a 1 σ radius of 0.°21) with no clear cutoff at high energies and emitting photons up to 210 TeV. We model the multiwavelength observations for the region around HESS J1809-193 using a time-dependent leptonic model and a lepto-hadronic model. Our model indicates that both scenarios could explain the observed data within the region of HESS J1809-193.

The Astrophysical JournalVol. 972(1)
Universidad Autónoma del Estado de Hidalgo (MX), Michigan Technological University (US), University of Seoul (KR), Los Alamos National Laboratory (US), University of Wisconsin–Madison (US), Universidad Autónoma de la Ciudad de México (MX), University of New Mexico (US), Universidad Michoacana de San Nicolás de Hidalgo (MX), Friedrich-Alexander-Universität Erlangen-Nürnberg (DE), Shanghai Jiao Tong University (CN), Universidad de Guadalajara (MX), University of Utah (US), National Institute of Astrophysics, Optics and Electronics (MX), Universidad Politécnica de Pachuca (MX), Institute of Nuclear Physics, Polish Academy of Sciences (PL), Universidad Autónoma de Chiapas (MX), Max Planck Institute for Nuclear Physics (DE), Instituto Politécnico Nacional (MX), University of Maryland, College Park (US), Benemérita Universidad Autónoma de Puebla (MX), Temple University (US), Sungkyunkwan University (KR), Michigan State University (US), Universidad Nacional Autónoma de México (MX), Stanford University (US), Tecnológico de Monterrey (MX)
National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, Consejo Nacional de Ciencia y Tecnología, Generalitat Valenciana, Benemérita Universidad Autónoma de Puebla, Office of National Higher Education Science Research and Innovation Policy Council, Goddard Space Flight Center, Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México, Coordinación de la Investigación Científica, Institute for Cosmic Ray Research, University of Tokyo, Laboratory Directed Research and Development, Los Alamos National Laboratory
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Astrophysics and Cosmic Phenomena
1.98
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