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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

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Showing 2021Show all

5 papers · 1 filter

astro-ph.EP2021★ 10 cited

How the planetary eccentricity influences the pebble isolation mass

Raúl O. Chametla, Frédéric S. Masset, Clément Baruteau +1

We investigate the pebble isolation mass for a planet on a fixed eccentric orbit in its protoplanetary disc by conducting a set of 2D hydrodynamical simulations including dust turb…

astro-ph.EP2021★ 16 cited

Wide Dust Gaps in Protoplanetary Disks Induced by Eccentric Planets: A Mass-Eccentricity Degeneracy

Yi-Xian Chen, Zhuoxiao Wang, Ya-Ping Li +2

The tidal perturbation of embedded protoplanets on their natal disks has been widely attributed to be the cause of gap-ring structures in sub-mm images of protoplanetary disks arou…

astro-ph.EP2021★ 19 cited

Observational signatures of eccentric Jupiters inside gas cavities in protoplanetary discs

Clément Baruteau, Gaylor Wafflard-Fernandez, Romane Le Gal +4

Predicting how a young planet shapes the gas and dust emission of its parent disc is key to constraining the presence of unseen planets in protoplanetary disc observations. We inve…

astro-ph.EP2021★ 55 cited

A dusty filament and turbulent CO spirals in HD135344B-SAO206462

Simon Casassus, Valentin Christiaens, Miguel Carcamo +16

Planet-disc interactions build up local pressure maxima that may halt the radial drift of protoplanetary dust, and pile it up in rings and crescents. ALMA observations of the HD135…

astro-ph.EP2021★ 9 cited

Observational constraints on the formation and evolution of Neptune-class exoplanets

M. Deleuil, D. Pollacco, C. Baruteau +2

Among exoplanets, the small-size population constitutes the dominant one, with a diversity of properties and compositions ranging from rocky to gas dominated envelope. While a larg…