141 citations · 760 across the 47 of their papers we have counts for
9 papers · 1 filter
Dust destruction and survival in the Cassiopeia A reverse shock
F. D. Priestley, M. Arias, M. J. Barlow +1
Core-collapse supernovae (CCSNe) produce large () masses of dust, and are potentially the primary source of dust in the Universe, but much of this dus…
The impact of metallicity-dependent dust destruction on the dust-to-metals ratio in galaxies
F. D. Priestley, I. De Looze, M. J. Barlow
The ratio of the mass of interstellar dust to the total mass of metals (the dust-to-metals/DTM ratio) tends to increase with metallicity. This can be explained by the increasing ef…
The JCMT BISTRO Survey: An 850/450m Polarization Study of NGC 2071IR in OrionB
A-Ran Lyo, Jongsoo Kim, Sarah Sadavoy +143
We present the results of simultaneous 450 m and 850 m polarization observations toward the massive star forming region NGC 2071IR, a target of the BISTRO (B-fields in Star-F…
The origin of a universal filament width in molecular clouds
F. D. Priestley, A. P. Whitworth
Filamentary structures identified in far-infrared observations of molecular clouds are typically found to have full-widths at half-maximum pc. However, the physical exp…
A systematic bias in fitting the surface-density profiles of interstellar filaments
Anthony Whitworth, Felix Priestley, Doris Arzoumanian
The surface-density profiles of dense filaments, in particular those traced by dust emission, appear to be well fit with Plummer profiles, i.e. Sigma(b)=Sigma_B+Sigma_O{1+[b/w_O]^2…
Molecular line signatures of cloud-cloud collisions
F. D. Priestley, A. P. Whitworth
Collisions between interstellar gas clouds are potentially an important mechanism for triggering star formation. This is because they are able to rapidly generate large masses of d…