Journal Article

PUBDB-2025-04857

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png An In-depth Study of Gamma Rays from the Starburst Galaxy M82 with VERITAS

Acharyya, A. ; Adams, C. B. ; Bangale, P. ; Bartkoske, J. T. ; Benbow, W. ; Buckley, J. H. ; Chen, Y. ; Christiansen, J. L. ; Chromey, A. J. ; Duerr, A. ; Errando, M. ; Godoy, M. E. ; Falcone, A. ; Feldman, S. ; Feng, Q. ; Foote, J. ; Fortson, L. ; Furniss, A. ; Hanlon, W. ; Hanna, D. ; Hervet, O. ; Hinrichs, C. E. ; Holder, J. ; Humensky, T. B. ; Jin, W. ; Johnson, M. N. ; Kaaret, P. ; Kertzman, M. ; Kherlakian, M. ; Kieda, D. ; Kleiner, T. K.DESY* ; Korzoun, N. ; Krennrich, F. ; Kumar, S. ; Lang, M. J. ; Lundy, M. ; Maier, G.DESY* ; Millard, M. J. ; Mooney, C. L. ; Moriarty, P. ; Mukherjee, R. ; Ning, W. ; Brien, S. Ó. ; Ong, R. A. ; Pohl, M.DESY* ; Pueschel, E.DESY* ; Quinn, J. ; Rabinowitz, P. L. ; Ragan, K. J. ; Reynolds, P. T. ; Ribeiro, D. ; Roache, E. ; Sadeh, I.DESY* ; Saha, L. ; Santander, M. ; Sembroski, G. H. ; Shang, R. ; Splettstoesser, M. ; Tak, D. ; Talluri, A. K. ; Tucci, J. V. ; Vassiliev, V. V. ; Williams, D. A. ; Wong, S. L. ; Woo, J. ; VERITAS Collaboration (Collaboration author)

2025
Institute of Physics Publ. London

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Please use a persistent id in citations: doi:10.3847/1538-4357/adab71  doi:10.3204/PUBDB-2025-04857

Report No.: arXiv:2501.09998

Abstract: Assuming Galactic cosmic rays originate in supernovae and the winds of massive stars, starburst galaxies should produce very-high-energy (VHE; E > 100 GeV) gamma-ray emission via the interaction of their copious quantities of cosmic rays with the large reservoirs of dense gas within the galaxies. Such VHE emission was detected by VERITAS from the starburst galaxy M82 in 2008–09. An extensive, multiyear campaign followed these initial observations, yielding a total of 254 hr of good-quality VERITAS data on M82. Leveraging modern analysis techniques and the larger exposure, these VERITAS data show a more statistically significant VHE signal (∼6.5 standard deviations, σ). The corresponding photon spectrum is well fit by a power law (Γ = 2.3 ± 0.3$_{stat}$ ± 0.2$_{sys}$), and the observed integral flux is F (>450 GeV) = (3.2 ± 0.6$_{stat}$ ± 0.6$_{sys}$) × 10$^{−13}$ cm$^{−2}$ s$^{−1}$, or ∼0.4% of the Crab Nebula flux above the same energy threshold. The improved VERITAS measurements, when combined with various multiwavelength data, enable modeling of the underlying emission and transport processes. A purely leptonic scenario is found to be a poor representation of the gamma-ray spectral energy distribution (SED). A lepto-hadronic scenario with cosmic rays following a power-law spectrum in momentum (index s ≃ 2.25) and with significant bremsstrahlung below 1 GeV provides a good match to the observed SED. The synchrotron emission from the secondary electrons indicates that efficient nonradiative losses of cosmic-ray electrons may be related to advective escape from the starburst core.

Note: 15 pages, 7 figures; Accepted for the publication in The Astrophysical Journal (ApJ)

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Contributing Institute(s):

1. VERITAS (Z_VER)

Research Program(s):

1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)

Experiment(s):

1. Very Energetic Radiation Imaging Telescope Array System

Appears in the scientific report 2025

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Linked articles:

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Preprint Acharyya, A. ; Adams, C. B. ; Bangale, P. ; et al
An In-depth Study of Gamma Rays from the Starburst Galaxy M82 with VERITAS
[10.3204/PUBDB-2025-04905]     Files  Fulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS

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