activity
20162026
most citedDiscovery of a planetary-mass companion within the gap of the transition disk around PDS 70

700 citations · 2.7k across the 64 of their papers we have counts for

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Showing astro-ph.SRShow all

10 papers · 1 filter

astro-ph.SR2024★ 4 cited

Astrometric and photometric characterization of Tel B combining two decades of observations

P. H. Nogueira, C. Lazzoni, A. Zurlo +11

Tel is an 18 Myr system with a 2.09 M A-type star and an M7-M8 brown dwarf companion, Tel B, separated by 4.2'' (208 au). High-contrast imaging campaigns over 20…

astro-ph.SR2022★ 9 cited

Updated orbital monitoring and dynamical masses for nearby M-dwarf binaries

Per Calissendorff, Markus Janson, Laetitia Rodet +26

Young M-type binaries are particularly useful for precise isochronal dating by taking advantage of their extended pre-main sequence evolution. Orbital monitoring of these low-mass…

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.SR2020★ 9 cited

Investigating three Sirius-like systems with SPHERE

R. Gratton, V. D'Orazi, T. A. Pacheco +61

Sirius-like systems are wide binaries composed of a white dwarf (WD) and a companion of a spectral type earlier than M0. The WD progenitor evolves in isolation, but its wind during…

astro-ph.SR2020★ 10 cited

The disk of 2MASS 15491331-3539118 = GQ Lup C as seen by HST and WISE

C. Lazzoni, R. Gratton, J. M. Alcalà +7

Very recently, a second companion on wider orbit has been discovered around GQ Lup. This is a low-mass accreting star partially obscured by a disk seen at high inclination. If dete…

astro-ph.SR2020★ 19 cited

2MASS J15491331-3539118: a new low-mass wide companion of the GQ Lup system

J. M. Alcalá, F. Z. Majidi, S. Desidera +14

Substellar companions at wide separation around stars hosting planets or brown dwarfs (BDs) yet close enough for their formation in the circumstellar disc are of special interest.…