CARAVEO, PATRIZIAPATRIZIACARAVEO2020-11-032020-11-0320182405-6014http://hdl.handle.net/20.500.12386/28135According to standard theoretical interpretations, in neutron stars’ magnetospheres particles are accelerated along the magnetic field lines where the highly-magnetized surrounding o ers the ideal conditions to make them radiate high-energy gamma-rays (E > 100 MeV) that bear the timing signature of their parent neutron star.ELETTRONICOenArticle10.1016/j.nuclphysbps.2018.07.0152-s2.0-85055317864000466262900015https://www.sciencedirect.com/science/article/pii/S2405601418301020?via%3Dihub2018NPPP..297...96CFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation