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researcher

A. Bevan

16 papers hereh-index 9343 citations23 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author3
  • middle author9
  • last author1

Across the 14 of 16 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR10
  • astro-ph.GA4
  • astro-ph.HE1
  • hep-ex1
same name
  • A. Bevan — 150 papers, h 30
  • A. Bevan — 132 papers, h 46
  • A. Bevan — 96 papers, h 75
  • A. Bevan — 44 papers, h 40
  • A. Bevan — 41 papers, h 6
  • A. Bevan — 5 papers, h 5

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20122023
most citedModelling supernova line profile asymmetries to determine ejecta dust masses: SN 1987A from days 714 to 3604

95 citations · 534 across the 16 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.GA2019

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…

astro-ph.SR2019★ 81 cited

Dust survival rates in clumps passing through the Cas A reverse shock I: results for a range of clump densities

Florian Kirchschlager, Franziska D. Schmidt, M. J. Barlow +3

The reverse shock in the ejecta of core-collapse supernovae is potentially able to destroy newly formed dust material. In order to determine dust survival rates, we have performed…

astro-ph.HE2019★ 45 cited

The dust content of the Crab Nebula

I. De Looze, M. J. Barlow, R. Bandiera +7

We have modelled the near-infrared to radio images of the Crab Nebula with a Bayesian SED model to simultaneously fit its synchrotron, interstellar and supernova dust emission. We…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.