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 …

Supernovae are considered as prime sources of dust in space. Observations of local
supernovae over the past couple of decades have detected the presence of dust in …

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 …

Supernova (SN) explosions are crucial engines driving the evolution of galaxies by shock
heating gas, increasing the metallicity, creating dust, and accelerating energetic particles. In …

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 …

High Angular Resolution ALMA Images of Dust and Molecules in the SN 1987A Ejecta -
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Supernova (SN) 1987A is the nearest supernova in∼ 400 yr. Using the JWST MIRI Medium
Resolution Spectrograph, we spatially resolved the ejecta, equatorial ring (ER), and outer …

The discovery with the Herschel Space Observatory of bright far-infrared and submm
emission from the ejecta of the core-collapse supernova SN 1987A has been interpreted as …

We study the formation of molecules and dust clusters in the ejecta of solar metallicity, Type
II-P supernovae (SNe) using a chemical kinetic approach. We follow the evolution of …

Supernovae (SNe) generate hot gas in the interstellar medium (ISM), help setting the ISM
structure, and support the driving of outflows. It is important to resolve the hot gas generation …