When I started working on my PhD project on X-ray spectroscopy of supernova remnants in
1995, one of the things that I missed was a good textbook covering the various aspects of …

Collisionless shock waves in supernova remnants and the solar wind heat electrons less
effectively than they heat ions, as is predicted by kinetic simulations. However, the values of …

Since the day of its explosion, SN 1987A (SN87A) was closely monitored with the aim to
study its evolution and to detect its central compact relic. The detection of neutrinos from the …

Context. Massive stars end their lives in catastrophic supernova (SN) explosions. Key
information on the explosion processes and on the progenitor stars can be extracted from …

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 …

Since the day of its explosion, supernova (SN) 1987A has been closely monitored to study
its evolution and to detect its central compact relic. In fact, the formation of a neutron star is …

X-ray observations of shock-heated plasmas, such as those found in supernova remnants
(SNRs), often exhibit features of temperature and ionization nonequilibrium. For accurate …

Based on observations with the Chandra X-ray Observatory, we present the latest spectral
evolution of the X-ray remnant of SN 1987A (SNR 1987A). We present a high-resolution …

This white paper was prepared by members of the XRISM Science Team for the benefit of
the general astronomical community. This paper describes the capabilities of XRISM, offers …

Electromagnetic turbulence and ion kinetics in counterstreaming plasmas hold great
significance in laboratory astrophysics, such as turbulence field amplification and particle …