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 …

There is a wealth of data on live, undecayed 60 Fe (t 1/2= 2.6 Myr) in deep-sea deposits, the
lunar regolith, cosmic rays, and Antarctic snow, which is interpreted as originating from the …

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

We present photometry and spectroscopy of the slowly evolving superluminous Type IIn
supernova (SN) 2015da. SN 2015da is extraordinary for its very high peak luminosity, and …

Dust associated with various stellar sources in galaxies at all cosmic epochs remains a
controversial topic, particularly whether supernovae play an important role in dust …

The expanding ejecta of supernova remnants (SNRs) are believed to form dust in dense
clumps of gas. Before the dust can be expelled into the interstellar medium and contribute to …

Dust from core-collapse supernovae (CCSNe), specifically Type IIP SNe, has been
suggested to be a significant source of the dust observed in high-redshift galaxies. CCSNe …

We report evidence of dust formation in the cold, dense shell behind the ejecta-circumstellar
medium (CSM) interaction in the Type Ia (SNIa) SN2018evt three years after the explosion …

We live in a dynamic star-forming galaxy, and as a result the solar neighborhood changes
constantly. One of the most spectacular events that inevitably occurs is the explosion of a …

GW170817 represents the first observed binary neutron star merger event by humanity. The
observation of GW170817 has identified the correlation between Kilonova, gravitational …