395 citations · 3.3k across the 129 of their papers we have counts for
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XMM-Newton observation of the supernova remnant Kes 78 (G32.8-0.1): Evidence for shock-cloud interaction
M. Miceli, A. Bamba, S. Orlando +4
The Galactic supernova remnant Kes 78 is surrounded by dense molecular clouds, whose projected position overlaps with the extended HESS gamma-ray source HESS J1852-000. The X-ray e…
Origin of asymmetries in X-ray emission lines from the blast wave of the 2014 outburst of nova V745 Sco
S. Orlando, J. J. Drake, M. Miceli
The symbiotic nova V745 Sco was observed in outburst on 2014 February 6. Its observations by the Chandra X-ray Observatory at days 16 and 17 have revealed a spectrum characterized…
Formation of X-ray emitting stationary shocks in magnetized protostellar jets
S. Ustamujic, S. Orlando, R. Bonito +3
X-ray observations of protostellar jets show evidence of strong shocks heating the plasma up to temperatures of a few million degrees. In some cases, the shocked features appear to…
Detailed study of SNR G306.3-0.9 using XMM-Newton and Chandra observations
J. A. Combi, F. García, A. E. Suárez +3
We used combined data from XMM-Newton and Chandra observatories to study the X-ray morphology of SNR G306.3-0.9. A spatially-resolved spectral analysis was used to obtain physical…
Modeling the shock-cloud interaction in SN 1006: unveiling the origin of nonthermal X-ray and gamma-ray emission
Marco Miceli, Salvatore Orlando, Victor Pereira +9
The supernova remnant SN 1006 is a source of high-energy particles and its southwestern limb is interacting with a dense ambient cloud, thus being a promising region for gamma-ray…
XMM-Newton Large Program on SN1006 - II: Thermal Emission
Jiang-Tao Li, Anne Decourchelle, Marco Miceli +2
Based on the XMM-Newton large program on SN1006 and our newly developed spatially resolved spectroscopy tools (Paper~I), we study the thermal emission from ISM and ejecta of SN1006…
Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: The role of post-explosion anisotropies of ejecta
S. Orlando, M. Miceli, M. L. Pumo +1
The remnants of core-collapse supernovae (SNe) have complex morphologies that may reflect asymmetries and structures developed during the progenitor SN explosion. Here we investiga…
Modeling non-thermal emission from stellar bow shocks
V. Pereira, J. López-Santiago, M. Miceli +2
Runaway O- and early B-type stars passing throughout the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serv…