395 citations · 3.3k across the 129 of their papers we have counts for
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Role of ejecta clumping and back-reaction of accelerated cosmic rays in the evolution of supernova remnants
S. Orlando, F. Bocchino, M. Miceli +2
The thermal structure of the post-shock region of a young supernova remnant (SNR) is heavily affected by two main physical effects, the back-reaction of accelerated cosmic rays (CR…
Overionization in X-ray spectra: a new paradigm for Mixed-Morphology SNRs
Marco Miceli
Mixed-morphology SNRs are characterized by a shell-like radio emission, a centrally peaked X-ray morphology, and by interaction with molecular clouds. Many models have been propose…
X-ray emission from protostellar jet HH 154: the first evidence of a diamond shock?
R. Bonito, S. Orlando, M. Miceli +3
X-ray emission from about ten protostellar jets has been discovered and it appears as a feature common to the most energetic jets. Although X-ray emission seems to originate from s…
Constraints on local interstellar magnetic field from non-thermal emission of SN1006
F. Bocchino, S. Orlando, M. Miceli +1
The synchrotron radio morphology of bilateral supernova remnants depends on the mechanisms of particle acceleration and on the viewing geometry. However, unlike X-ray and -ray m…
Widespread nanoflare variability detected with Hinode/XRT in a solar active region
Sergio Terzo, Fabio Reale, Marco Miceli +3
It is generally agreed that small impulsive energy bursts called nanoflares are responsible for at least some of the Sun's hot corona, but whether they are the explanation for most…
Suzaku Detection of Diffuse Hard X-Ray Emission outside Vela X
Satoru Katsuda, Koji Mori, Robert Petre +9
Vela X is a large, 3x2 degrees, radio-emitting pulsar wind nebula (PWN) powered by the Vela pulsar in the Vela supernova remnant. Using four Suzaku/XIS observations pointed just ou…