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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 2015Show all

5 papers · 1 filter

astro-ph.EP2015★ 98 cited

Gas and dust hydrodynamical simulations of massive lopsided transition discs - II. Dust concentration

Clément Baruteau, Zhaohuan Zhu

We investigate the dynamics of large dust grains in massive lopsided transition discs via 2D hydrodynamical simulations including both gas and dust. Our simulations adopt a ring-li…

astro-ph.EP2015★ 65 cited

Gas and dust hydrodynamical simulations of massive lopsided transition discs - I. Gas distribution

Zhaohuan Zhu, Clément Baruteau

Motivated by lopsided structures observed in some massive transition discs, we have carried out 2D numerical simulations to study vortex structure in massive discs, including the e…

astro-ph.EP2015★ 29 cited

Modelling circumbinary protoplanetary disks: I. Fluid simulations of the Kepler-16 and 34 systems

S. Lines, Z. M. Leinhardt, C. Baruteau +2

The Kepler mission's discovery of a number of circumbinary planets orbiting close (a_p < 1.1 au) to the stellar binary raises questions as to how these planets could have formed gi…

astro-ph.EP2015★ 36 cited

Protoplanetary disks including radiative feedback from accreting planets

Matias Montesinos, Jorge Cuadra, Sebastian Perez +2

While recent observational progress is converging on the detection of compact regions of thermal emission due to embedded protoplanets, further theoretical predictions are needed t…

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…