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A. D. de Souza

35 papers hereh-index 201.7k citations67 works total

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

author position
  • first author4
  • middle author16
  • last author7

Across the 27 of 35 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR24
  • astro-ph.IM4
  • gr-qc4
  • astro-ph3
same name
  • A. D. de Souza — 2 papers, h 0
  • A. D. de Souza — 2 papers, h 3
  • A. D. de Souza — 1 paper, h 0
  • A. D. de Souza — 1 paper, h 13

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
20032026
most citedThe spinning-top Be star Achernar from VLTI-VINCI

216 citations · 797 across the 33 of their papers we have counts for

collaborators
Showing 2010Show all

3 papers · 1 filter

astro-ph.SR2010★ 21 cited

Differential rotation in rapidly rotating early-type stars. I. Motivations for combined spectroscopic and interferometric studies

J. Zorec, Y. Fremat, A. Domiciano de Souza +7

Since the external regions of the envelopes of rapidly rotating early-type stars are unstable to convection, a coupling may exist between the convection and the internal rotation.…

astro-ph.SR2010★ 4 cited

Fast ray-tracing algorithm for circumstellar structures (FRACS) I. Algorithm description and parameter-space study for mid-IR interferometry of B[e] stars

Gilles Niccolini, Philippe Bendjoya, Armando Domiciano De Souza

The physical interpretation of spectro-interferometric data is strongly model-dependent. On one hand, models involving elaborate radiative transfer solvers are too time consuming i…

astro-ph.SR2010★ 13 cited

Fast ray-tracing algorithm for circumstellar structures (FRACS). II. Disc parameters of the B[e] supergiant CPD-57° 2874 from VLTI/MIDI data

Armando Domiciano De Souza, Philippe Bendjoya, Gilles Niccolini +6

B[e] supergiants are luminous, massive post-main sequence stars exhibiting non-spherical winds, forbidden lines, and hot dust in a disc-like structure. The physical properties of t…

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