Details

Autor(en) / Beteiligte

• Albert, A.
• Alfaro, R.
• Alvarez, C.
• Arteaga-Velázquez, J. C.
• Rojas, D. Avila
• Solares, H. A. Ayala
• Babu, R.
• Belmont-Moreno, E.
• Blochwitz, C.
• Caballero-Mora, K. S.
• Capistrán, T.
• Carramiñana, A.
• Casanova, S.
• Chaparro-Amaro, O.
• Cotti, U.
• Cotzomi, J.
• De la Fuente, E.
• de León, C.
• de León, S. Coutiño
• Diaz Hernandez, R.
• Dingus, B. L.
• DuVernois, M. A.
• Durocher, M.
• Díaz-Vélez, J. C.
• Engel, K.
• Espinoza, C.
• Fan, K. L.
• Fang, K.
• Fraija, N.
• García-González, J. A.
• Garfias, F.
• González, M. M.
• Goodman, J. A.
• Harding, J. P.
• Hernandez, S.
• Hinton, J.
• Huang, D.
• Hueyotl-Zahuantitla, F.
• Hüntemeyer, P.
• Iriarte, A.
• Joshi, V.
• Lara, A.
• Lee, W. H.
• Linnemann, J. T.
• Longinotti, A. L.
• Luis-Raya, G.
• Lundeen, J.
• Malone, K.
• Marandon, V.
• Martinez, O.
• Martínez-Castro, J.
• Matthews, J. A.
• Miranda-Romagnoli, P.
• Morales-Soto, J. A.
• Moreno, E.
• Mostafá, M.
• Nayerhoda, A.
• Nellen, L.
• Newbold, M.
• Nisa, M. U.
• Noriega-Papaqui, R.
• Omodei, N.
• Peisker, A.
• Araujo, Y. Pérez
• Pérez-Pérez, E. G.
• Rho, C. D.
• Rosa-González, D.
• Ruiz-Velasco, E.
• Salazar-Gallegos, D.
• Greus, F. Salesa
• Sandoval, A.
• Serna-Franco, J.
• Smith, A. J.
• Son, Y.
• Springer, R. W.
• Tibolla, O.
• Tollefson, K.
• Torres, I.
• Torres-Escobedo, R.
• Turner, R.
• Ureña-Mena, F.
• Villaseñor, L.
• Wang, X.
• Willox, E.
• Zepeda, A.
• Zhou, H.
• Chomiuk, L.
• Aydi, E.
• Li, K. L.
• Metzger, B. D.
• Vurm, I.

Titel

γ-Ray Emission from Classical Nova V392 Per: Measurements from Fermi and HAWC

Ist Teil von

• The Astrophysical journal, 2022-12, Vol.940 (2), p.141

Ort / Verlag

Philadelphia: The American Astronomical Society

Erscheinungsjahr

2022

Link zum Volltext

Quelle

EZB-FREE-00999 freely available EZB journals

Beschreibungen/Notizen

• Abstract This paper reports on the γ -ray properties of the 2018 Galactic nova V392 Per, spanning photon energies ∼0.1 GeV–100 TeV by combining observations from the Fermi Gamma-ray Space Telescope and the HAWC Observatory. As one of the most rapidly evolving γ -ray signals yet observed for a nova, GeV γ -rays with a power-law spectrum with an index Γ = 2.0 ± 0.1 were detected over 8 days following V392 Per’s optical maximum. HAWC observations constrain the TeV γ -ray signal during this time and also before and after. We observe no statistically significant evidence of TeV γ -ray emission from V392 Per, but present flux limits. Tests disfavor the extension of the Fermi Large Area Telescope spectrum to energies above 5 TeV by 2 standard deviations (95%) or more. We fit V392 Per’s GeV γ -rays with hadronic acceleration models, incorporating optical observations, and compare the calculations with HAWC limits.