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F. Millour

150 papers hereh-index 343.8k citations287 works total

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

author position
  • sole author5
  • first author24
  • middle author94
  • last author1

Across the 124 of 150 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR62
  • astro-ph.IM34
  • astro-ph.GA21
  • astro-ph17
  • astro-ph.EP10
  • astro-ph.CO4
same name
  • F. Millour — 11 papers

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
20052026
most citedMapping the radial structure of AGN tori

156 citations · 3k across the 144 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.CO2013★ 59 cited

Evidence for a receding dust sublimation region around a supermassive black hole

Makoto Kishimoto, Sebastian F. Hoenig, Robert Antonucci +6

The near-IR emission in Type 1 AGNs is thought to be dominated by the thermal radiation from dust grains that are heated by the central engine in the UV/optical and are almost at t…

astro-ph.SR2013★ 16 cited

Evidence of an asymmetrical Keplerian disk in the Brγ and He I emission lines around the Be star HD 110432

Philippe Stee, A. Meilland, Ph. Bendjoya +6

Context. HD 110432 was classified as a "γCas X-ray analog" since it has similar peculiar X-ray and optical characteristics, i.e. a hard-thermal X-ray variable emission and an optic…

astro-ph.SR2013★ 5 cited

The binary Be star δ Scorpii at high spectral and spatial resolution : II The circumstellar disk evolution after the periastron

Anthony Meilland, Philippe Stee, Alain Spang +3

Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar disk that is responsible for the observed infrared (IR) excess and emission lines. The influen…

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