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researcher

D M-A Meyer

10 papers here

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

author position
  • first author4
  • middle author4
  • last author1

Across the 9 of 10 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR7
  • astro-ph.HE2
  • astro-ph.GA1
ORCID 0000-0001-8258-9813

identity via Semantic Scholar / OpenAlex

activity
20122023
most citedOn the existence of accretion-driven bursts in massive star formation

146 citations · 448 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

2 papers · 1 filter

astro-ph.HE2023★ 20 cited

The sculpting of rectangular and jet-like morphologies in supernova remnants by anisotropic equatorially-confined progenitor stellar winds

P. F. Velazquez, D. M. -A. Meyer, A. Chiotellis +5

Thermonuclear and core-collapse supernova remnants (SNRs) are the nebular leftovers of defunct stars. Their morphology and emission properties provide insights into the evolutionar…

astro-ph.HE2022★ 17 cited

Rectangular core-collapse supernova remnants: application to Puppis A

D. M. -A. Meyer, P. F. Velazquez, O. Petruk +9

Core-collapse supernova remnants are the gaseous nebulae of galactic interstellar media (ISM) formed after the explosive death of massive stars. Their morphology and emission prope…

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