119 citations · 893 across the 33 of their papers we have counts for
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Deep XMM-Newton Observations Reveal the Origin of Recombining Plasma in the Supernova Remnant W44
Hiromichi Okon, Takaaki Tanaka, Hiroyuki Uchida +8
Recent X-ray studies revealed over-ionized recombining plasmas (RPs) in a dozen mixed-morphology (MM) supernova remnants (SNRs). However, the physical process of the over-ionizatio…
Hydrodynamic simulations unravel the progenitor-supernova-remnant connection in SN 1987A
S. Orlando, M. Ono, S. Nagataki +8
(Abridged) We aim at linking the dynamical and radiative properties of the remnant of SN 1987A to the geometrical and physical characteristics of the parent aspherical SN explosion…
Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A
Masaomi Ono, Shigehiro Nagataki, Gilles Ferrand +5
We perform three-dimensional hydrodynamic simulations of aspherical core-collapse supernovae focusing on the matter mixing in SN 1987A. The impacts of four progenitor (pre-supernov…
Spatially resolved X-ray study of supernova remnants that host magnetars: Implication of their fossil field origin
Ping Zhou, Jacco Vink, Samar Safi-Harb +1
Magnetars are regarded as the most magnetized neutron stars in the Universe. Aiming to unveil what kinds of stars and supernovae can create magnetars, we have performed a state-of-…
A stellar flare-coronal mass ejection event revealed by X-ray plasma motions
C. Argiroffi, F. Reale, J. J. Drake +6
Coronal mass ejections (CMEs), often associated with flares, are the most powerful magnetic phenomena occurring on the Sun. Stars show magnetic activity levels up to 10^4 times hig…
Collisionless shock heating of heavy ions in SN 1987A
Marco Miceli, Salvatore Orlando, David N. Burrows +6
Astrophysical shocks at all scales, from those in the heliosphere up to the cosmological shock waves, are typically "collisionless", because the thickness of their jump region is m…