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researcher

A. Bevan

8 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 author1
  • middle author5

Across the 7 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
  • astro-ph.GA3
  • astro-ph.HE1
same name
  • A. Bevan — 60 papers, h 75
  • A. Bevan — 43 papers, h 40
  • A. Bevan — 32 papers, h 46
  • A. Bevan — 16 papers, h 6
  • A. Bevan — 10 papers, h 30
  • A. Bevan — 2 papers, h 2

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
20182021
most citedThe dust content of the Crab Nebula

45 citations · 90 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2021

The dust mass in Cassiopeia A from infrared and optical line flux differences

Maria Niculescu-Duvaz, Michael J. Barlow, Antonia Bevan +2

The large quantities of dust that have been found in a number of high redshift galaxies have led to suggestions that core-collapse supernovae (CCSNe) are the main sources of their…

astro-ph.GA2020★ 11 cited

Constraining early-time dust formation in core-collapse supernovae

F. D. Priestley, A. Bevan, M. J. Barlow +1

There is currently a severe discrepancy between theoretical models of dust formation in core-collapse supernovae (CCSNe), which predict ≳0.01 M⊙​ of ejecta dust form…

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…

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