Dust is a ubiquitous feature of the cosmos, impinging directly or indirectly on most fields of
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …

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 …

The dust-to-stellar mass ratio (M dust/M⋆) is a crucial, albeit poorly constrained, parameter
for improving our understanding of the complex physical processes involved in the …

Dust-obscured star formation has dominated the cosmic history of star formation, since z≃ 4.
However, the recent finding of significant amount of dust in galaxies out to z≃ 8 has opened …

Modelling the red–blue asymmetries seen in the broad emission lines of core-collapse
supernovae (CCSNe) is a powerful technique to quantify total dust mass formed in the ejecta …

We present a study of the dust associated with the core-collapse supernova SN 1995N.
Infrared emission detected 14–15 yr after the explosion was previously attributed to …

We present the mid-infrared (MIR) light curves (LC) of 10 superluminous supernovae
(SLSNe) at z< 0.12 based on WISE data at 3.4 and 4.6 m. Three of them, including PS15br …

Large discrepancies are found between observational estimates and theoretical predictions
when exploring the characteristics of dust formed in the ejecta of a core-collapse …

Context. The dense Galactic environment is a large reservoir of interstellar dust. Therefore,
this region represents a perfect laboratory to study the properties of cosmic dust grains. X …

The unusual extinction curves of SN 2010jl provide an excellent opportunity to investigate
the properties of dust formed by core-collapse supernovae. By using a series of dust models …