Munar-Adrover, PerePereMunar-AdroverPIANO, GiovanniGiovanniPIANOSabatini, S.S.SabatiniTAVANI, MARCOMARCOTAVANILUCARELLI, FabrizioFabrizioLUCARELLIVERRECCHIA, FrancescoFrancescoVERRECCHIAPITTORI, CarlottaCarlottaPITTORI2021-01-262021-01-262017978-0-7354-1456-30094-243Xhttp://hdl.handle.net/20.500.12386/30005The AGILE satellite has been proven to be an excellent tool to study transient gamma-ray sources since it entered in a spinning operational mode in 2009. Thanks to its scanning capabilities it observes the whole sky every few hours. Several new interesting systems were discovered, such as AGL J2241+4454 in 2010, probably associated to the mysterious black-hole high-mass X-ray binary MWC 656. With a state of the art PSF and sensitivity in the 100 MeV – 1 GeV energy range, AGILE studied this system in order to identify new periods of gamma-ray activity that could be associated to the binary, and found a total of 10 flares spanning from 2008 until 2013. AGILE studied also the Cygnus region, finding evidence of a new recent gamma-ray flare from the microquasar Cygnus X-3, with a flux of ∼ 2×10−8 ph cm−2 s, during a state transition phase in the bright high-soft X-ray state. Also Cygnus X-1 was detected in the past by AGILE, although both systems are very different and show different behaviour.STAMPAenConference paper10.1063/1.49689192-s2.0-85010931178000399207800034https://aip.scitation.org/doi/abs/10.1063/1.49689192017AIPC.1792d0015MFIS/05 - ASTRONOMIA E ASTROFISICA