Abstract
M87 is a giant radio galaxy located in the Virgo Cluster, known to be a very high energy (VHE) gamma-ray source. As radio galaxies are considered the misaligned low-redshift counterparts of blazars, they are excellent laboratories for testing AGN emission models. M87 has been detected and monitored by Fermi-LAT and several atmospheric Cherenkov telescopes. Recently, the HAWC Collaboration presented marginal evidence of 4.5-year TeV gamma-ray emission from this object. The HAWC data has the potential to constrain the average VHE emission of sources of complex behavior, like M87, for which the physical origin of the VHE gamma-ray emission is still uncertain. We fitted a lepto-hadronic scenario to the broadband spectral energy distribution of M87 to model its non-flaring VHE emission using HAWC data.
Recommended Citation
F. Ureña-Mena and A. Carramiñana and A. L. Longinotti and D. Rosa-González and A. U. Abeysekara and A. Albert and R. Alfaro and C. Alvarez and J. D. Álvarez and J. R. Angeles Camacho and J. C. Arteaga-Velázquez and K. P. Arunbabu and D. Avila Rojas and H. A. Ayala Solares and R. Babu and V. Baghmanyan and A. S. Barber and J. Becerra Gonzalez and E. Belmont-Moreno and S. Y. BenZvi and D. Berley and C. Brisbois and K. S. Caballero-Mora and T. Capistran and A. Carraminana and S. Casanova and O. Chaparro-Amaro and U. Cotti and J. Cotzomi and S. Coutino de Leon and E. De la Fuente and C. de Leon and L. Diaz-Cruz and R. Diaz Hernandez and J. C. Diaz-Velez and B. L. Dingus and M. Durocher and M. A. DuVernois and R. W. Ellsworth and K. Engel and C. Espinoza and K. L. Fan and K. Fang and M. Fernandez Alonso and B. Fick and H. Fleischhack and J. L. Flores and N. I. Fraija and D. Garcia and J. A. Garcia-Gonzalez and J. L. Garcia-Luna and G. Garcia-Torales and F. Garfias and G. Giacinti and H. Goksu and M. M. Gonzalez and J. A. Goodman and J. P. Harding and S. Hernandez and I. Herzog and J. Hinton and B. Hona and D. Huang and F. Hueyotl-Zahuantitla and C. M. Hui and B. Humensky and P. Huntemeyer and A. Iriarte and A. Jardin-Blicq and H. Jhee and V. Joshi and D. Kieda and G. J. Kunde and S. Kunwar and A. Lara and J. Lee and W. H. Lee and D. Lennarz and H. Leon Vargas and J. Linnemann and A. L. Longinotti and R. Lopez-Coto and G. Luis-Raya and J. Lundeen and K. Malone and V. Marandon and O. Martinez and I. Martinez-Castellanos and H. Martinez-Huerta and J. Martinez-Castro and J. A. Matthews and J. McEnery and P. Miranda-Romagnoli and J. A. Morales-Soto and E. Moreno and M. Mostafa and A. Nayerhoda and L. Nellen and M. Newbold and M. U. Nisa and R. Noriega-Papaqui and L. Olivera-Nieto and N. Omodei and A. Peisker and Y. Perez Araujo and E. G. Perez-Perez and C. D. Rho and C. Riviere and D. Rosa-Gonzalez and E. Ruiz-Velasco and J. Ryan and H. Salazar and F. Salesa Greus and A. Sandoval and M. Schneider and H. Schoorlemmer and J. Serna-Franco and G. Sinnis and A. J. Smith and R. W. Springer and P. Surajbali and I. Taboada and M. Tanner and K. Tollefson and I. Torres and R. Torres-Escobedo and R. Turner and F. Urena-Mena and L. Villasenor and X. Wang and I. J. Watson and T. Weisgarber and F. Werner and E. Willox and J. Wood and G. B. Yodh and A. Zepeda and H. Zhou, "Modeling The Non-flaring VHE Emission From M87 As Detected By The HAWC Gamma Ray Observatory," Proceedings of Science, vol. 395, article no. 841, Sissa Medialab Srl, Mar 2022.
The definitive version is available at https://doi.org/10.48550/arXiv.2108.01048
Department(s)
Physics
International Standard Serial Number (ISSN)
1824-8039
Document Type
Article - Conference proceedings
Document Version
Citation
File Type
text
Language(s)
English
Rights
© 2025 Sissa Medialab Srl, All rights reserved.
Publication Date
18 Mar 2022
Comments
National Science Foundation, Grant PRODEP-SEP UDG-CA-499