Aims: We study the production of dust in Type II-P supernova by coupling the gas-phase chemistry to the dust nucleation and condensation phases. We consider two supernova progenitor masses with homogeneous and clumpy ejecta to assess the chemical type and quantity of dust that forms. Grain size distributions are derived as a function of post-explosion time. Methods: The chemistry of the gas phase and the simultaneous formation of dust clusters are described by a chemical network. The formation of key species (CO, SiO) and dust clusters of silicates, alumina, silica, metal carbides and sulphides, pure metals, and amorphous carbon is considered. The master equations describing the chemistry of the nucleation phase are coupled to a dust cond...
We study the dust evolution in the supernova remnant Cassiopeia A. We follow the processing of dust ...
Context. Core collapse supernovae (CCSNe) are important sources of interstellar dust, which are pote...
Supernovae are considered as prime sources of dust in space. Observations of local supernovae over t...
Aims. We study the production of dust in Type II-P supernova ejecta by coupling the gas-phase chemis...
Aims. We study the chemistry of the Type IIb supernova ejecta that led to the Cas A supernova remnan...
Aims. We study the chemistry of the type IIb supernova ejecta, which led to the Cas A supernova rem...
We study the formation of molecules and dust clusters in the ejecta of solar metallicity, Type II-P ...
At redshift z>~ 5, Type II supernovae (SNeII) are the only known dust sources with evolutionary time...
Observations of local supernovae over the past couple of decades have reported the presence of dust ...
Large discrepancies are found between observational estimates and theoretical predictions when explo...
We study the formation of molecular precursors to dust in the ejecta of Population III supernovae (P...
We present a novel investigation of dust synthesis in the ejecta of supernovae of zero metallicity p...
The amount and size of dust formed in the ejecta of core-collapse supernovae (CCSNe) and injected in...
Emerging from the Big Bang, the Universe contained hydrogen, helium, and lithium. Heavier elements w...
Large discrepancies are found between observational estimates and theoretical predictions when explo...
We study the dust evolution in the supernova remnant Cassiopeia A. We follow the processing of dust ...
Context. Core collapse supernovae (CCSNe) are important sources of interstellar dust, which are pote...
Supernovae are considered as prime sources of dust in space. Observations of local supernovae over t...
Aims. We study the production of dust in Type II-P supernova ejecta by coupling the gas-phase chemis...
Aims. We study the chemistry of the Type IIb supernova ejecta that led to the Cas A supernova remnan...
Aims. We study the chemistry of the type IIb supernova ejecta, which led to the Cas A supernova rem...
We study the formation of molecules and dust clusters in the ejecta of solar metallicity, Type II-P ...
At redshift z>~ 5, Type II supernovae (SNeII) are the only known dust sources with evolutionary time...
Observations of local supernovae over the past couple of decades have reported the presence of dust ...
Large discrepancies are found between observational estimates and theoretical predictions when explo...
We study the formation of molecular precursors to dust in the ejecta of Population III supernovae (P...
We present a novel investigation of dust synthesis in the ejecta of supernovae of zero metallicity p...
The amount and size of dust formed in the ejecta of core-collapse supernovae (CCSNe) and injected in...
Emerging from the Big Bang, the Universe contained hydrogen, helium, and lithium. Heavier elements w...
Large discrepancies are found between observational estimates and theoretical predictions when explo...
We study the dust evolution in the supernova remnant Cassiopeia A. We follow the processing of dust ...
Context. Core collapse supernovae (CCSNe) are important sources of interstellar dust, which are pote...
Supernovae are considered as prime sources of dust in space. Observations of local supernovae over t...