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LIST OF RELEVANT REFEREED PUBLICATIONS

Publications based on hydrodynamic and MHD models using either the FLASH or the PLUTO code. The numerical simulations have been performed on a variety of supercomputers, including those hosted at CINECA (Italy), BSC (Spain), CINES (France), the Linux clusters hosted at the HPC facility SCAN of INAF-OAPA (Italy), and the Grid Infrastructure of Consorzio COMETA (Italy).

  • SOLAR PHYSICS

    • MHD modeling of coronal loops: the transition region throat
      Guarrasi M., Reale F., Orlando S., Mignone A., Klimchuk J.A. 2014, A&A 564, id.A48

    • MHD-modeling of the propagation of a coronal mass ejection
      Pagano P., Reale F., Orlando S., Peres G. 2007, A&A 464, 753

    • Modeling magnetohydrodynamics and non-equilibrium SoHO/UVCS line emission of CME shocks
      Pagano P., Raymond J.C., Reale F., Orlando S. 2008, A&A 481, 835

    • MHD modeling of coronal loops: injection of high-speed chromospheric flows
      Petralia A., Reale F., Orlando S., Klimchuk J.A. 2014, A&A 567, A70

    • Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: Magnetic Channelling
      Petralia A., Reale F., Orlando S., Testa P. 2016, ApJ 832, id.2

    • Magnetic shuffling of coronal downdrafts
      Petralia A., Reale F., Orlando S. 2017, A&A 598, id.L8

    • Nonequilibrium of Ionization and the Detection of Hot Plasma in Nanoflare-heated Coronal Loops
      Reale F., Orlando S. 2008, ApJ 684, 715

    • Post-flare UV light curves explained with thermal instability of loop plasma
      Reale F., Landi E., Orlando S. 2012, ApJ 746, 18

    • Bright hot impacts by erupted fragments falling back on the Sun: a template for stellar accretion
      Reale F., Orlando S., Testa P., Peres G., Landi E., Schrijver C.J. 2013, Science 341, 251

    • Bright hot impacts by erupted fragments falling back on the Sun: UV redshifts in stellar accretion
      Reale F., Orlando S., Testa P., Landi E., Schrijver C.J. 2014, ApJ 797, L5

    • 3D MHD modeling of twisted coronal loops
      Reale F., Orlando S., Guarrasi M., Mignone A., Peres G., Hood A.W., Priest E.R. 2016, ApJ 830, id.21

  • YOUNG STELLAR OBJECTS AND PROTOSTELLAR JETS

    • The X-ray Emission Mechanism in the Protostellar Jet HH 154
      Bonito R., Orlando S., Peres G., Favata F., Rosner R. 2004, A&A 424, L1

    • X-rays from protostellar jets: emission from continuous flows
      Bonito R., Orlando S., Peres G., Favata F., Rosner R. 2007, A&A 462, 645

    • Generation of radiative knots in a randomly pulsed protostellar jet I. Dynamics and energetics
      Bonito R., Orlando S., Peres G., Eisloffel J., Miceli M., Favata F. 2010, A&A 511, A42

    • Generation of radiative knots in a randomly pulsed protostellar jet II. X-ray emission
      Bonito R., Orlando S., Miceli M., Eisloffel J., Peres G., Favata F. 2010, A&A 517, A68

    • X-ray emission from protostellar jet HH 154: the first evidence of a diamond shock?
      Bonito R., Orlando S., Miceli M., Peres G., Micela G., Favata F. 2011, ApJ 737, id. 54

    • Magnetohydrodynamic modeling of the accretion shocks in classical T Tauri stars: the role of local absorption on the X-ray emission
      Bonito R., Orlando S., Argiroffi C., Miceli M., Peres G., Matsakos T., Stehle C., Ibgui L. 2014, ApJ 795, L34

    • Impacts of fragmented accretion streams onto Classical T Tauri Stars: UV and X-ray emission lines
      Colombo S., Orlando S., Peres G., Argiroffi C., Reale F. 2016, A&A 594, id.A93

    • Hydrodynamic Modeling of Accretion Impacts in Classical T Tauri Stars: Radiative Heating of the Pre-shock Plasma
      Costa G., Orlando S., Peres G., Argiroffi C., Bonito R., Reale F. 2017, A&A 597, A1

    • X-ray emission from stellar jets by collision against high-density molecular clouds: an application to HH 248
      Lopez-Santiago J., Bonito R., Orellana M., Miceli M., Orlando S., Ustamujic S., Albacete-Colombo F.J., de Castro E., Gomez de Castro Ana Ines 2015, ApJ 806, 53

    • YSO accretion shocks: magnetic, chromospheric or stochastic flow effects can suppress fluctuations of X-ray emission
      Matsakos T., Chieze J.-P., Stehle' C., Gonzalez M., Ibgui L., de Sa' L., Lanz T., Orlando S., Bonito R., Argiroffi C., Reale F., Peres G. 2013, A&A 557, A69

    • X-ray emitting MHD accretion shocks in classical T Tauri stars. Case for moderate to high plasma-beta values
      Orlando S., Sacco G.G., Argiroffi C., Reale F., Peres G., Maggio A. 2010, A&A 510, A71

    • Mass accretion to young stars triggered by flaring activity in circumstellar disks
      Orlando S., Reale F., Peres G., Mignone A. 2011, MNRAS 415, 3380

    • Radiative accretion shocks along nonuniform stellar magnetic fields in classical T Tauri
      Orlando S., Bonito R., Argiroffi C., Reale F., Peres G., Miceli M., Matsakos T., Stehle' C., Ibgui L., de Sa L., Chie`ze J.P., Lanz T. 2013, A&A 559, id.A127

    • Mass Accretion Processes in Young Stellar Objects: Role of Intense Flaring Activity
      Orlando S., Reale F., Peres G., Mignone A. 2014, Acta Polytechnica CTU Proceedings 1(1), 108

    • Laboratory unraveling of matter accretion in young stars
      Revet G., Chen S.A., Bonito R., Khiar B., Filippov E., Argiroffi C., Higginson D.P., Orlando S., Béard J., Blecher M., Borghesi M., Burdonov K., Khaghani D., Naughton K., Pépin H., Portugall O., Riquier R., Rodriguez R., Ryazantsev S.N., Skobelev I.Yu., Soloviev A., Willi O., Pikuz S., Ciardi A., Fuchs J. 2017, Science Advances 3, e1700982

    • X-ray emission from dense plasma in CTTSs: Hydrodynamic modeling of the accretion shock
      Sacco G.G., Argiroffi C., Orlando S., Maggio A., Peres G., Reale F. 2008, A&A 491, L17

    • On the observability of T Tauri accretion shocks in the X-ray band
      Sacco G.G., Orlando S., Argiroffi C., Maggio A., Peres G., Reale F., Curran R.L. 2010, A&A 522, A55

    • Formation of X-ray emitting stationary shocks in magnetized protostellar jets
      Ustamujic S., Orlando S., Bonito R., Miceli M., Gomez de Castro A.I., Lopez-Santiago J. 2016, A&A 596, A99

  • CATACLYSMIC VARIABLES AND NOVA OUTBURSTS

    • Accretion disk coronae of intermediate polar cataclysmic variables. 3D magnetohydrodynamic modelling and thermal X-ray emission
      Barbera E., Orlando S., Peres G. 2017, A&A 600, A105

    • The early blast wave of the 2010 explosion of U Scorpii
      Drake J.J., Orlando S. 2010, ApJ 720, L195

    • Three-dimensional modeling of the asymmetric blast wave from the 2006 outburst of RS Ophiuchi: Early X-ray emission
      Orlando S., Drake J.J., Laming J.M. 2009, A&A 493, 1049

    • Modeling the 2010 blast wave of the symbiotic-like nova V407 Cygni
      Orlando S., Drake J.J. 2012, MNRAS 419, 2329

    • Origin of asymmetries in X-ray emission lines from the blast wave of the 2014 outburst of nova V745 Sco
      Orlando S., Drake J.J., Miceli M. 2017, MNRAS 464, 5003

  • SUPERNOVA REMNANTS

    • Constraints on local interstellar magnetic field from non-thermal emission of SN1006
      Bocchino F., Orlando S., Miceli M., Petruk O. 2011, A&A 531, A129

    • Shock-cloud interaction in the Vela SNR II. Hydrodynamic model
      Miceli M., Reale F., Orlando S., Bocchino F. 2006, A&A 458, 213

    • Hydrodynamic modelling of ejecta shrapnel in the Vela supernova remnant
      Miceli M., Orlando S., Reale F., Bocchino F., Peres G. 2013, MNRAS 430, 2864

    • Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and gamma-ray emission
      Miceli M., Orlando S., Pereira V., Acero F., Katsuda K., Decourchelle A., Winkler F.P., Bonito R., Reale F., Peres G., Li J., Dubner G. 2016, A&A 593, id.A26

    • Crushing of Interstellar Gas Clouds in Supernova Remnants I. The Role of Thermal Conduction and Radiative Losses
      Orlando S., Peres G., Reale F., Bocchino F., Rosner R., Plewa T., Siegel A. 2005, A&A 444, 505

    • Crushing of Interstellar Gas Clouds in Supernova Remnants II. X-ray Emission
      Orlando S., Bocchino F., Peres G., Reale F., Plewa T., Rosner R. 2006, A&A 457, 545

    • On the Origin of Asymmetries in Bilateral Supernova Remnants
      Orlando S., Bocchino F., Reale F., Peres G., Petruk O. 2007, A&A 470, 927

    • The importance of magnetic-field-oriented thermal conduction in the interaction of SNR shocks with interstellar clouds
      Orlando S., Bocchino F., Reale F., Peres G., Pagano P. 2008, ApJ 678, 274

    • Modeling SNR shock waves expanding through the magnetized inhomogeneous interstellar medium
      Orlando S., Bocchino F., Miceli M., Reale F., Peres G. 2009, Il Nuovo Cimento C 32, 45

    • Observability and diagnostics in the X-ray band of shock-cloud interactions in supernova remnants
      Orlando S., Bocchino F., Miceli M., Zhou X., Reale F., Peres G. 2010, A&A 514, A29

    • Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton gamma-ray morphology of SNRs
      Orlando S., Petruk O., Bocchino F., Miceli M. 2011, A&A 526, A129

    • Role of Ejecta Clumping and Back-reaction of Accelerated Cosmic Rays in the Evolution of Type Ia Supernova Remnants
      Orlando S., Bocchino F., Miceli M., Petruk O., Pumo M.L. 2012, ApJ 749, 156

    • Supernova 1987A: a Template to Link Supernovae to Their Remnants
      Orlando S., Miceli M., Pumo M.L., Bocchino F. 2015, ApJ 810, 168

    • Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: The role of post-explosion anisotropies of ejecta
      Orlando S., Miceli M., Pumo M.L., Bocchino F. 2016, ApJ 822, id. 22

    • Linking gamma-ray spectra of supernova remnants to the cosmic ray injection properties in the aftermath of supernovae
      Petruk O., Orlando S., Miceli M., Bocchino F. 2017, A&A 605, A110

    • Unveiling the spatial structure of the overionized plasma in the supernova remnant W49B
      Zhou X., Miceli M., Bocchino F., Orlando S., Chen Y. 2011, MNRAS 415, 244