We present a detailed stellar population analysis of 11 bright (H< 26.6) galaxies at z= 9–11
(three spectroscopically confirmed) to constrain the chemical enrichment and growth of …

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 …

We complement the parsec data base of stellar evolutionary tracks with new models of
massive stars, from the pre-main-sequence phase to the central carbon ignition. We …

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 …

We present an empirical analysis of the properties of dust-continuum emission in a sample
of 17 galaxies in the early Universe (4< z< 8) with well-sampled far-infrared spectral energy …

Aims. We model the synthesis of molecules and dust in the inner wind of the oxygen-rich
Mira-type star IK Tau by considering the effects of periodic shocks induced by the stellar …

The recent discovery of high-redshift dusty galaxies implies a rapid dust enrichment of their
interstellar medium (ISM). To interpret these observations, we run a cosmological simulation …

The nearby Supernova 1987A was accompanied by a burst of neutrino emission, which
indicates that a compact object (a neutron star or black hole) was formed in the explosion …

Supernova (SN) explosions have been sought for decades as a possible source of dust in
the Universe, providing the seeds of galaxies, stars, and planetary systems. SN 1987A offers …