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  1. OA@INAF
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Browsing by Author MORLINO, Giovanni


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Showing results 24 to 42 of 42 < previous 
Issue DateTitleAuthor(s)Fulltext
2019Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layoutAcharyya, A.; Agudo, I.; Angüner, E. O.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Alves Batista, R.; Amans, J. -P.; AMATI, LORENZO , et alopen
2017Multi-messenger Observations of a Binary Neutron Star MergerAbbott, B. P.; Abbott, R.; Abbott, T. D.; Acernese, F.; Ackley, K.; Adams, C.; Adams, T.; Addesso, P.; Adhikari, R. X.; Adya, V. B., et alopen
2019Multi-Messenger Physics with the Pierre Auger ObservatoryThe Pierre Auger Collaboration; Aab, A.; Abreu, P.; AGLIETTA, MARCO ; Albuquerque, I. F. M.; Albury, J. M.; Allekotte, I.; Almela, A.; Alvarez Castillo, J.; Alvarez-Muñiz, J., et alopen
2020New high-frequency radio observations of the Cygnus Loop supernova remnant with the Italian radio telescopesLORU, SARA ; PELLIZZONI, ALBERTO PAOLO ; EGRON, ELISE MARIE JEANNE ; INGALLINERA, Adriano ; MORLINO, GIOVANNI ; Celli, S; UMANA, Grazia Maria Gloria ; TRIGILIO, CORRADO ; LETO, PAOLO ; Iacolina, M N, et alopen
2015Non-linear Cosmic Ray propagation close to the acceleration siteNava, Lara ; Gabici, S.; Marcowith, A.; MORLINO, GIOVANNI ; Ptuskin, V.open
2016Non-linear diffusion of cosmic rays escaping from supernova remnants - I. The effect of neutralsNava, Lara ; Gabici, S.; Marcowith, A.; MORLINO, GIOVANNI ; Ptuskin, V. S.open
2018Numerical simulations of mass loading in the tails of bow-shock pulsar-wind nebulaeOlmi, Barbara ; BUCCIANTINI, NICCOLO' ; MORLINO, GIOVANNI open
2018Observation of inclined EeV air showers with the radio detector of the Pierre Auger ObservatoryAab, A.; Abreu, P.; AGLIETTA, MARCO ; Albuquerque, I. F. M.; Albury, J. M.; Allekotte, I.; Almela, A.; Alvarez Castillo, J.; Alvarez-Muñiz, J.; Anastasi, G. A., et alopen
2016On the radial distribution of Galactic cosmic raysRecchia, S.; Blasi, P.; MORLINO, GIOVANNI open
2018Origin of the Cosmic Ray Galactic Halo Driven by Advected Turbulence and Self-Generated WavesEvoli, Carmelo; Blasi, Pasquale; MORLINO, GIOVANNI ; Aloisio, Robertoopen
2019Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger ObservatoryAab, A.; Abreu, P.; AGLIETTA, MARCO ; Albuquerque, I. F. M.; Albury, J. M.; Allekotte, I.; Almela, A.; Alvarez Castillo, J.; Alvarez-Muñiz, J.; Anastasi, G. A., et alopen
2017Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7-3946Acero, F.; Aloisio, R.; Amans, J.; AMATO, Elena ; ANTONELLI, Lucio Angelo ; Aramo, C.; Armstrong, T.; Arqueros, F.; Asano, K.; Ashley, M., et alopen
2017Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger ObservatoryAlbert, A.; André, M.; Anghinolfi, M.; Ardid, M.; Aubert, J. -J.; Aublin, J.; Avgitas, T.; Baret, B.; Barrios-Martí, J.; Basa, S., et alopen
2018Self-generated cosmic-ray confinement in TeV halos: Implications for TeV γ -ray emission and the positron excessEvoli, Carmelo; Linden, Tim; MORLINO, GIOVANNI open
2016Spectra of accelerated particles at supernova shocks in the presence of neutral hydrogen: the case of TychoMORLINO, GIOVANNI ; Blasi, P.open
2019Supernova remnants in clumpy media: particle propagation and gamma-ray emissionSilvia Celli; MORLINO, GIOVANNI ; Stefano Gabici; Felix Aharonianopen
2019Understanding the Origin and Impact of Relativistic Cosmic Particles with Very-High-Energy Gamma-raysHolder, Jamie; AMATO, Elena ; BANDIERA, Rino ; Bird, R.; BULGARELLI, ANDREA ; Dwarkadas, V. V.; Giglietto, N.; Goldoni, P.; Hinton, J.; Hnatyk, B., et alopen
2018What causes the ionization rates observed in molecular clouds? The role of cosmic ray protons and electronsV. H. M. Phan; MORLINO, GIOVANNI ; S. Gabiciopen
2016XIPE: the x-ray imaging polarimetry explorerSOFFITTA, PAOLO ; Bellazzini, R.; Bozzo, E.; Burwitz, V.; Castro-Tirado, A.; Costa, E.; Courvoisier, T.; Feng, H.; Gburek, S.; Goosmann, R., et alopen
Showing results 24 to 42 of 42 < previous 

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