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Albert, A. ; Alfaro, R. ; Alvarez, C. ; Arteaga-Velázquez, J. C. ; Avila Rojas, D. ; Ayala Solares, H. A. ; Babu, R. ; Belmont-Moreno, E. ; Brisbois, C. ; Caballero-Mora, K. S. ; et al ( , Physical Review Letters)
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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. ; et al ( , The Astrophysical Journal)
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 evolvingγ -ray signals yet observed for a nova, GeVγ -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 TeVγ -ray signal during this time and also before and after. We observe no statistically significant evidence of TeVγ -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 GeVγ -rays with hadronic acceleration models, incorporating optical observations, and compare the calculations with HAWC limits. -
Albert, A. ; Alfaro, R. ; Alvarez, C. ; Arceo, R. ; Arteaga-Velázquez, J. C. ; Avila Rojas, D. ; Ayala Solares, H. A. ; Belmont-Moreno, E. ; BenZvi, S. Y. ; Brisbois, C. ; et al ( , Physical Review D)
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Alfaro, R. ; Alvarez, C. ; Álvarez, J. D. ; Arceo, R. ; Arteaga-Velázquez, J. C. ; Avila Rojas, D. ; Ayala Solares, H. A. ; Barber, A. S. ; Becerril, A. ; Belmont-Moreno, E. ; et al ( , Physical Review D)
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Abeysekara, A. U. ; Alfaro, R. ; Alvarez, C. ; Álvarez, J. D. ; Arceo, R. ; Arteaga-Velázquez, J. C. ; Ayala Solares, H. A. ; Barber, A. S. ; Baughman, B. M. ; Bautista-Elivar, N. ; et al ( , Physical Review D)