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Dispersion and Rotation Measures from the Ejecta of Compact Binary Mergers: Clue to the Progenitors of Fast Radio Bursts
Revisiting the evolution of non-radiative supernova remnants: a hydrodynamical-informed parametrization of the shock positions
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Turbulent mixing of r-process elements in the Milky Way
Dust survival rates in clumps passing through the Cas A reverse shock – I. Results for a range of clump densities
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A catalogue of Galactic supernova remnants in the far-infrared: revealing ejecta dust in pulsar wind nebulae
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Where does galactic dust come from?
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Pyroclastic Blowout: Dust Survival in Isolated versus Clustered Supernovae
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Iron and Silicate Dust Growth in the Galactic Interstellar Medium: Clues from Element Depletions
A Massive Shell of Supernova-formed Dust in SNR G54.1+0.3
Tea Temim, Eli Dwek, Richard G. Arendt, Kazimierz J. Borkowski, Stephen P. Reynolds, Patrick Slane, Joseph D. Gelfand and John C. Raymond The Astrophysical Journal 836(1) 129 (2017) https://doi.org/10.3847/1538-4357/836/1/129
Galaxy Evolution Studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA): The Power of IR Spectroscopy
L. Spinoglio, A. Alonso-Herrero, L. Armus, et al. Publications of the Astronomical Society of Australia 34 (2017) https://doi.org/10.1017/pasa.2017.48
The dust mass in Cassiopeia A from a spatially resolvedHerschelanalysis
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A cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia A
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Hydrodynamic ablation of protoplanetary discs via supernovae
Chemical enrichment of the pre-solar cloud by supernova dust grains
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IRON: A KEY ELEMENT FOR UNDERSTANDING THE ORIGIN AND EVOLUTION OF INTERSTELLAR DUST