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20202026
most citedA wide-orbit giant planet in the high-mass b Centauri binary system

52 citations · 413 across the 29 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.EP2021★ 52 cited

A wide-orbit giant planet in the high-mass b Centauri binary system

Markus Janson, Raffaele Gratton, Laetitia Rodet +24

Planet formation occurs around a wide range of stellar masses and stellar system architectures. An improved understanding of the formation process can be achieved by studying it ac…

astro-ph.EP2021★ 21 cited

Signs of late infall and possible planet formation around DR Tau using VLT/SPHERE and LBTI/LMIRCam

D. Mesa, C. Ginski, R. Gratton +31

Context. Protoplanetary disks around young stars often contain substructures like rings, gaps, and spirals that could be caused by interactions between the disk and forming planets…

astro-ph.GA2021★ 37 cited

Unveiling the star formation history of the Upper Scorpius association through its kinematics

Vito Squicciarini, Raffaele Gratton, Mariangela Bonavita +1

Stellar associations can be discerned as overdensities of sources not only in the physical space but also in the velocity space. The common motion of their members, gradually erode…

astro-ph.SR2021★ 20 cited

New binaries from the SHINE survey

M. Bonavita, R. Gratton, S. Desidera +67

We present the multiple stellar systems observed within the SpHere INfrared survey for Exoplanet (SHINE). SHINE searched for substellar companions to young stars using high contras…

astro-ph.EP2021★ 9 cited

Limits on the presence of planets in systems with debris disks: HD 92945 and HD 107146

D. Mesa, S. Marino, M. Bonavita +38

Recent observations of resolved cold debris disks at tens of au have revealed that gaps could be a common feature in these Kuiper belt analogues. Such gaps could be evidence for th…

astro-ph.EP2021★ 31 cited

BEAST begins: Sample characteristics and survey performance of the B-star Exoplanet Abundance Study

Markus Janson, Vito Squicciarini, Philippe Delorme +20

While the occurrence rate of wide giant planets appears to increase with stellar mass at least up through the A-type regime, B-type stars have not been systematically studied in la…