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C. Baruteau

82 papers hereh-index 323.5k citations108 works total

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

author position
  • first author15
  • middle author52
  • last author6

Across the 73 of 82 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP59
  • astro-ph.SR16
  • astro-ph.GA3
  • astro-ph2
  • astro-ph.CO1
  • astro-ph.IM1
same name
  • C. Baruteau — 15 papers, h 4
  • C. Baruteau — 6 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
20072026
most citedA torque formula for non-isothermal Type I planetary migration - II. Effects of diffusion

526 citations · 5k across the 79 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2024

A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk

Olivier Berné, Emilie Habart, Els Peeters +143

Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiati…

astro-ph.GA2015★ 7 cited

Very Large Telescope observations of Gomez's Hamburger: Insights into a young protoplanet candidate

O. Berne, A. Fuente, E. Pantin +8

Planets are thought to form in the gas and dust disks around young stars. In particular, it has been proposed that giant planets can form through the gravitational instability of m…

astro-ph.GA2010★ 132 cited

Binaries migrating in a gaseous disk: Where are the Galactic center binaries?

C. Baruteau, J. Cuadra, D. N. C. Lin

The massive stars in the Galactic center inner arcsecond share analogous properties with the so-called Hot Jupiters. Most of these young stars have highly eccentric orbits, and wer…

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