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).
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SOLAR PHYSICS
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MHD modeling of coronal loops: the
transition region throat
Guarrasi M., Reale F., Orlando S., Mignone A., Klimchuk J.A. 2014,
A&A 564, A48
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MHD-modeling of the propagation of a coronal mass
ejection
Pagano P., Reale F., Orlando S., Peres G. 2007, A&A 464, 753
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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
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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
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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
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Magnetic shuffling of coronal
downdrafts Petralia A., Reale F., Orlando S. 2017,
A&A 598, L8
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Guided flows in coronal magnetic flux
tubes Petralia A., Reale F., Testa P. 2018, A&A
609, A18
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Nonequilibrium of Ionization and the Detection
of Hot Plasma in Nanoflare-heated Coronal Loops
Reale F., Orlando S. 2008, ApJ 684, 715
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Post-flare UV light curves explained
with thermal instability of loop plasma Reale F.,
Landi E., Orlando S. 2012, ApJ 746, 18
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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
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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
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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
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X-Ray Flare Oscillations Track Plasma
Sloshing along Star-disk Magnetic Tubes in the Orion Star-forming
Region Reale F., Lopez-Santiago J., Flaccomio E.,
Petralia A., Sciortino S. 2018, ApJ 856, id.51
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YOUNG STELLAR OBJECTS AND PROTOSTELLAR JETS
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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
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X-rays from protostellar jets:
emission from continuous flows
Bonito R., Orlando S., Peres G., Favata F., Rosner R.
2007, A&A 462, 645
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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
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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
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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
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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
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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, A93
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New view of the corona of classical T
Tauri stars: Effects of flaring activity in circumstellar disks
Colombo S., Orlando S., Peres G., Reale F., Argiroffi
C., Bonito R., Ibgui L., Stehle C. 2019, A&A 624, A50
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Effects of radiation in accretion regions
of classical T Tauri stars. Pre-heating of accretion column in
non-LTE regime Colombo S., Ibgui L., Orlando S.,
Rodriguez R., Espinosa G., Gonzalez M., Stehle C., de Sa L.,
Argiroffi C., Bonito R., Peres G. 2019, A&A 629, L9
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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
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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
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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
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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
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Mass accretion to young stars triggered by
flaring activity in circumstellar disks
Orlando S., Reale F., Peres G., Mignone A. 2011, MNRAS 415, 3380
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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, A127
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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
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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
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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
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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
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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
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Structure of X-ray emitting jets close to
the launching site: from embedded to disk-bearing sources
Ustamujic S., Orlando S., Bonito R., Miceli M.,
Gomez de Castro A.I. 2018, A&A 615, A124
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Predicting the time variation of radio
emission from MHD simulations of a flaring T-Tauri star
Waterfall C.O.G., Browning P.K., Fuller G.A., Gordovskyy M., Orlando S.,
Reale F. 2020, MNRAS 496, 2715
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CATACLYSMIC VARIABLES AND NOVA OUTBURSTS
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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
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The early blast wave of the 2010 explosion
of U Scorpii Drake J.J., Orlando S. 2010, ApJ
720, L195
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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
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Modeling the 2010 blast wave of the
symbiotic-like nova V407 Cygni Orlando S., Drake
J.J. 2012, MNRAS 419, 2329
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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
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SUPERNOVA REMNANTS
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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
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Indication of a Pulsar Wind Nebula in the
Hard X-Ray Emission from SN 1987A
Greco E., Miceli M., Orlando S., Olmi B., Bocchino F., Nagataki S.,
Ono M., Dohi A., Peres G. 2021, ApJL 908, id.L45
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Additional Evidence for a Pulsar Wind
Nebula in the Heart of SN 1987A from Multiepoch X-Ray Data and
MHD Modeling
Greco E., Miceli M., Orlando S., Olmi B., Bocchino F., Nagataki S.,
Sun L., Vink J., Sapienza V., Ono M., Dohi A., Peres G. 2022,
ApJ 931, id.132
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Shock-cloud interaction in the Vela SNR II.
Hydrodynamic model
Miceli M., Reale F., Orlando S., Bocchino F. 2006, A&A 458, 213
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Hydrodynamic modelling of ejecta
shrapnel in the Vela supernova remnant
Miceli M., Orlando S., Reale F., Bocchino F., Peres G. 2013,
MNRAS 430, 2864
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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, A26
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Collisionless shock heating of heavy ions
in SN 1987A Miceli M., Orlando S., Burrows D.N.,
Frank K.A., Argiroffi C., Reale F., Peres G., Petruk O., Bocchino F.
2019, Nature Astronomy 3, 236
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Matter Mixing in Aspherical Core-collapse
Supernovae: Three-dimensional Simulations with Single Star and
Binary Merger Progenitor Models for SN 1987A
Ono M., Nagataki S., Ferrand G.,Takahashi K., Umeda H., Yoshida T.,
Orlando S., Miceli M. 2019, ApJ 888, 111
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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
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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
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On the Origin of Asymmetries in
Bilateral Supernova Remnants
Orlando S., Bocchino F., Reale F., Peres G., Petruk O.
2007, A&A 470, 927
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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
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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
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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
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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
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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
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Supernova 1987A: a Template to Link
Supernovae to Their Remnants Orlando S., Miceli M.,
Pumo M.L., Bocchino F. 2015, ApJ 810, 168
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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
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3D MHD modeling of the expanding remnant
of SN 1987A. Role of magnetic field and non-thermal radio
emission Orlando S., Miceli M., Petruk O., Ono M.,
Nagataki S., Aloy M.A., Mimica P., Lee S.-H., Bocchino F., Peres G.,
Guarrasi M. 2019, A&A 622, A73
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Hydrodynamic simulations unravel the
progenitor-supernova-remnant connection in SN1987A
Orlando S., Ono M., Nagataki S., Miceli M., Umeda H., Ferrand G.,
Bocchino F., Petruk O., Peres G., Takahashi K., Yoshida T. 2020,
A&A 636, A22
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The fully developed remnant of a
neutrino-driven supernova. Evolution of ejecta structure and
asymmetries in SNR Cassiopeia A
Orlando S., Wongwathanarat A., Janka H.-T., Miceli M., Ono
M., Nagataki S., Bocchino F., Peres, G. 2021, A&A 645, A66
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Modeling particle acceleration and
non-thermal emission in supernova remnants
Orlando S., Miceli M., Ustamujic S., Tutone A., Greco E., Petruk O.,
Bocchino F., Peres G. 2021, New Astronomy 86, id.101566
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Evidence for past interaction with an
asymmetric circumstellar shell in the young SNR Cassiopeia A
Orlando S., Wongwathanarat A., Janka H.-T., Miceli M., Nagataki S.,
Ono M., Bocchino F., Vink J., Milisavljevic D., Patnaude D.J.,
Peres G. 2022, A&A 666, A2
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Connecting supernova remnants to their
parent supernovae
Orlando S., Miceli M., Bocchino F., Peres G. 2023, Mem. SAIt 93, 182
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Radio Evolution of Supernova Remnants
Including Non-linear Particle Acceleration: Insights from
Hydrodynamic Simulations Pavlović M.Z.,
Urošević D., Arbutina B., Orlando S., Maxted N., Filipović M.D.
2018, ApJ 852, id.84
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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
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Magneto-hydrodynamic simulations of young
supernova remnants and their energy-conversion phase
Petruk O., Kuzyo T., Orlando S., Pohl M., Brose R. 2021, MNRAS
505, 755
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Polarized radio emission unveils the
structure of the pre-supernova circumstellar magnetic field and
the radio emission in SN1987A
Petruk O., Beshley V., Orlando S., Bocchino F., Miceli M., Nagataki S.,
Ono M., Loru S., Pellizzoni A., Egron E. 2023, MNRAS 518, 6377
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Three-dimensional modeling from the
onset of the SN to the full-fledged SNR. Role of an initial ejecta
anisotropy on matter mixing
Tutone A., Orlando S., Miceli M., Ustamujic S., Ono M., Nagataki S.,
Ferrand G., Greco E., Peres G., Warren D.C., Bocchino F. 2020,
A&A 642, A67
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Modeling the mixed-morphology supernova
remnant IC 443
Ustamujic S., Orlando S., Greco E., Miceli M., Bocchino F., Tutone
A., Peres G. 2021, A&A 649, A14
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Modeling the remnants of core-collapse
supernovae from luminous blue variable stars
Ustamujic S., Orlando S., Miceli M., Bocchino F., Limongi M.,
Chieffi A., Trigilio C., Umana G., Bufano F., Ingallinera A., Peres
G. 2021, A&A 654, A167
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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
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NUMERICAL METHODS AND CODES
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Non-LTE radiation hydrodynamics in
PLUTO
Colombo S., Ibgui L., Orlando S., Rodriguez R., Espinosa G.,
Gonzalez M., Stehle C., Peres G. 2019, A&A 631, A41
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