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20142026
most citedKinematic detection of a planet carving a gap in a protoplanetary disc

187 citations · 1.7k across the 29 of their papers we have counts for

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9 papers · 1 filter

astro-ph.SR2020

The Carina High-Contrast Imaging Project for massive Stars (CHIPS) I. Methodology and proof of concept on QZ Car ( HD93206)

A. Rainot, M. Reggiani, H. Sana +13

Massive stars like company. However, low-mass companions have remained extremely difficult to detect at angular separations () smaller than 1" (~1000-3000 au considering typical…

astro-ph.SR2020★ 46 cited

The Ophiuchus DIsc Survey Employing ALMA (ODISEA). II. The effect of stellar multiplicity on disc properties

Alice Zurlo, Lucas A. Cieza, Sebastián Pérez +9

We present Adaptive Optics (AO) near infrared (NIR) observations using VLT/NACO and Keck/NIRC2 of ODISEA targets. ODISEA is an ALMA survey of the entire population of circumstellar…

astro-ph.SR2020★ 1 cited

Discovery of a low-mass companion embedded in the disk of the young massive star MWC 297 with VLT/SPHERE

M. Giulia Ubeira-Gabellini, Valentin Christiaens, Giuseppe Lodato +4

We report the discovery of a low-mass stellar companion around the young Herbig Be star MWC 297. We performed multi-epoch high-contrast imaging in the near infrared (NIR) with the…

astro-ph.SR2020★ 162 cited

Nine localised deviations from Keplerian rotation in the DSHARP circumstellar disks: Kinematic evidence for protoplanets carving the gaps

C. Pinte, D. J. Price, F. Menard +12

We present evidence for localised deviations from Keplerian rotation, i.e., velocity "kinks", in 8 of 18 circumstellar disks observed by the DSHARP program: DoAr 25, Elias 2-27, GW…

astro-ph.SR2019★ 187 cited

Kinematic detection of a planet carving a gap in a protoplanetary disc

C. Pinte, G. van der Plas, F. Menard +10

We still do not understand how planets form, or why extra-solar planetary systems are so different from our own solar system. But the last few years have dramatically changed our v…

astro-ph.SR2018★ 186 cited

Circumbinary, not transitional: On the spiral arms, cavity, shadows, fast radial flows, streamers and horseshoe in the HD142527 disc

Daniel J. Price, Nicolas Cuello, Christophe Pinte +13

We present 3D hydrodynamical models of the HD142527 protoplanetary disc, a bright and well studied disc that shows spirals and shadows in scattered light around a 100 au gas cavity…

astro-ph.SR2015★ 109 cited

A compact concentration of large grains in the HD142527 protoplanetary dust trap

Simon Casassus, Chris Wright, Sebastian Marino +11

A pathway to the formation of planetesimals, and eventually giant planets, may occur in concentrations of dust grains trapped in pressure maxima. Dramatic crescent-shaped dust conc…

astro-ph.SR2015★ 130 cited

Accretion kinematics through the warped transition disk in HD142527 from resolved CO(6-5) observations

Simon Casassus, Sebastian Marino, Sebastian Perez +10

The finding of residual gas in the large central cavity of the HD142527 disk motivates questions on the origin of its non-Keplerian kinematics, and possible connections with planet…

astro-ph.SR2014★ 35 cited

Spatially resolved HCN J=4--3 and CS J=7--6 emission from the disk around HD 142527

G. van der Plas, S. Casassus, F. Menard +4

The disk around HD 142527 attracts a lot of attention, amongst others because of its resolved (sub) mm dust continuum that is concentrated into a horseshoe-shape towards the north…