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E. di Folco

23 papers hereh-index 00 citations0 works total

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

author position
  • first author1
  • middle author20
  • last author2

Across the 23 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR9
  • astro-ph.EP8
  • astro-ph3
  • astro-ph.GA3
same name
  • E. Di Folco — 4 papers
  • E. Di Folco — 3 papers, h 9

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 · 1.3k across the 23 of their papers we have counts for

collaborators
Showing 2014Show all

4 papers · 1 filter

astro-ph.GA2014★ 29 cited

Circumbinary Ring, Circumstellar disks and accretion in the binary system UY Aurigae

Ya-Wen Tang, Anne Dutrey, Stephane Guilloteau +8

Recent exo-planetary surveys reveal that planets can orbit and survive around binary stars. This suggests that some fraction of young binary systems which possess massive circumbin…

astro-ph.SR2014★ 83 cited

The masses of young stars: CN as a probe of dynamical masses

S. Guilloteau, M. Simon, V. Piétu +4

Aims: We attempt to determine the masses of single or multiple young T Tauri and HAeBe stars from the rotation of their Keplerian disks. Methods:We used the IRAM PdBI interferomete…

astro-ph.SR2014★ 43 cited

GG Tau: the fifth element

E. Di Folco, A. Dutrey, J. -B. Le Bouquin +9

We aim at unveiling the observational imprint of physical mechanisms that govern planetary formation in young, multiple systems. In particular, we investigate the impact of tidal t…

astro-ph.EP2014★ 76 cited

Faint disks around classical T Tauri stars: small but dense enough to form planets?

V. Piétu, S. Guilloteau, E. di Folco +2

(abridged) Most Class II sources (of nearby star forming regions) are surrounded by disks with weak millimeter continuum emission. These "faint" disks may hold clues to the disk di…

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