368 citations · 10.3k across the 170 of their papers we have counts for
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Dust masses and grain size distributions of a sample of Galactic pulsar wind nebulae
F. D. Priestley, M. J. Barlow, I. De Looze +1
We calculate dust spectral energy distributions (SEDs) for a range of grain sizes and compositions, using physical properties appropriate for five pulsar wind nebulae (PWNe) from w…
Dust destruction by the reverse shock in the clumpy supernova remnant Cassiopeia A based on hydrodynamic simulations
Florian Kirchschlager, Franziska D. Schmidt, M. J. Barlow +3
Observations of the ejecta of core-collapse supernovae have shown that dust grains form in over-dense gas clumps in the expanding ejecta. The clumps are later subject to the passag…
The mass, location and heating of the dust in the Cassiopeia A supernova remnant
F. D. Priestley, M. J. Barlow, I. De Looze
We model the thermal dust emission from dust grains heated by synchrotron radiation and by particle collisions, under conditions appropriate for four different shocked and unshocke…