Abstract
The Cygnus Cocoon is the first gamma-ray superbubble powered by a massive stellar association, the OB2 association. It was postulated that the combined effects of the stellar winds of all the massive O-type stars of the OB2 association can accelerate the cosmic rays to PeV energy in the Cocoon. The conclusive proof of acceleration to PeV energy in the Cocoon will identify the stellar association as a PeV cosmic-ray accelerator, known as PeVatron. However, the Cocoon has been previously studied only up to 10 TeV. In this contribution, using 1343 days of High Altitude Water Cherenkov (HAWC) observatory data, we present the morphological and spectral study of the Cocoon above 1 TeV to beyond 100 TeV. The analysis at higher TeV energies reveals a softer spectrum compared to the GeV gamma-ray observation. This result suggests that the accelerator's efficiency decreases around hundreds of TeV, or after being accelerated, the highest-energy protons escape the region. The study above 10 TeV presented here demonstrates how CR accelerators operate in these extreme energies and how particle transport impacts high-energy emission.
Recommended Citation
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. Du Vernois 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. Mirando-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, "Particle Acceleration In The Cygnus Superbubble," Proceedings of Science, vol. 395, article no. 831, Sissa Medialab Srl, Mar 2022.
The definitive version is available at https://doi.org/10.48550/arXiv.2108.09348
Department(s)
Physics
Publication Status
Open Access
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