Marco Miceli
0000-0003-0876-8391
70 papers found
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Detailed study of SNR G306.3−0.9 usingXMM-NewtonandChandraobservations
XMM–Newtonlarge programme on SN1006 – II. Thermal emission
Modeling Snr Cassiopeia a From the Supernova Explosion to Its Current Age: The Role of Post-Explosion Anisotropies of Ejecta
Modeling nonthermal emission from stellar bow shocks
XMM-Newton large program on SN1006 - I. Methods and initial results of spatially resolved spectroscopy
An X-ray characterization of the central region of the supernova remnant G332.5-5.6
Supernova 1987a: A Template to Link Supernovae to Their Remnants
X-Ray Emission From Stellar Jets by Collision Against High-Density Molecular Clouds: An Application to Hh 248
Spatial Distribution of X-Ray Emitting Ejecta in Tycho̊squos SNR: Indications of Shocked Titanium
Spatial Distribution of X-Ray Emitting Ejecta in Tycho’s Snr: Indications of Shocked Titanium
Magnetohydrodynamic Modeling of the Accretion Shocks in Classical T Tauri Stars: The Role of Local Absorption in the X-Ray Emission
The loss-limited electron energy in SN 1006: Effects of the shock velocity and of the diffusion process
Shock-Cloud Interaction and Particle Acceleration in the Southwestern Limb of Sn 1006
Radiative accretion shocks along nonuniform stellar magnetic fields in classical T Tauri stars
Evidence of Non-thermal X-Ray Emission from HH 80
The shape of the cutoff in the synchrotron emission of SN 1006 observed with XMM-Newton
The northwestern ejecta knot in SN 1006
Hydrodynamic modelling of ejecta shrapnel in the Vela supernova remnant
Non-thermal processes in coronae and beyond
XMM-Newtonevidence of shocked ISM in SN 1006: indications of hadronic acceleration
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