The explosion of a supernova releases almost instantaneously about 10^ 51 51 ergs of
mechanic energy, changing irreversibly the physical and chemical properties of large …

Although it has faded by a factor of∼ 107, SN 1987A is still bright enough to be observed in
almost every band of the electromagnetic spectrum. Today, the bolometric luminosity of the …

The final evolution of stars in the mass range 70–140${\text {}}{M} _ {\odot} $ is explored.
Depending upon their mass loss history and rotation rates, these stars will end their lives as …

Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …

JCW had long wanted to write a new monograph on supernovae. Despite an immense
explosion in the literature and many review articles, there had not been one since that of …

We propose a semi-analytical model for the self-intersection of the fallback stream in tidal
disruption events (TDEs). When the initial periapsis is less than about 15 gravitational radii …

We present new Herschel photometric and spectroscopic observations of Supernova 1987A,
carried out in 2012. Our dedicated photometric measurements provide new 70 μm data and …

We propose a new extra but non-cosmological explanation for fast radio bursts (FRBs)
based on very young pulsars in supernova remnants. Within a few hundred years of a core …

High Angular Resolution ALMA Images of Dust and Molecules in the SN 1987A Ejecta -
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We report on a method, PUSH, for artificially triggering core-collapse supernova explosions
of massive stars in spherical symmetry. We explore basic explosion properties and calibrate …