par Liu, Qinrui;Aguilar Sanchez, Juan Antonio 
;Baur, Sebastian ;Iovine, Nadège ;Maris, Ioana Codrina ;Mockler, Daniela ;Raab, Christoph ;Renzi, Giovanni ;Toscano, Simona ; [et al.]
Référence Pos proceedings of science, 395, 1136
Publication Publié, 2022-03-01
;Baur, Sebastian ;Iovine, Nadège ;Maris, Ioana Codrina ;Mockler, Daniela ;Raab, Christoph ;Renzi, Giovanni ;Toscano, Simona ; [et al.]Référence Pos proceedings of science, 395, 1136
Publication Publié, 2022-03-01
Article révisé par les pairs
| Résumé : | X-ray binaries are long-standing source candidates of Galactic cosmic rays and neutrinos. The compact object in a binary system can be the site for cosmic-ray acceleration, while high-energy neutrinos can be produced by the interactions of cosmic rays in the jet of the compact object, the stellar wind, or the atmosphere of the companion star. We report a time-dependent study of high-energy neutrinos from X-ray binaries with IceCube using 7.5 years of muon neutrino data and X-ray observations. In the absence of significant correlation, we report upper limits on the neutrino fluxes from these sources and provide a comparison with theoretical predictions. |
