activity
20172025
most citedA highly settled disk around Oph 163131

138 citations · 542 across the 10 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2022138 cited

A highly settled disk around Oph 163131

M. Villenave, K. R. Stapelfeldt, G. Duchene +10

High dust density in the midplane of protoplanetary disks is favorable for efficient grain growth and can allow fast formation of planetesimals and planets, before disks dissipate.…

astro-ph.SR202131 cited

Circumbinary and circumstellar discs around the eccentric binary IRAS 04158+2805 -- a testbed for binary-disc interaction

Enrico Ragusa, Daniele Fasano, Claudia Toci +10

IRAS~04158+2805 has long been thought to be a very low mass T-Tauri star (VLMS) surrounded by a nearly edge-on, extremely large disc. Recent observations revealed that this source…

astro-ph.SR202122 cited

Probing protoplanetary disk evolution in the Chamaeleon II region

M. Villenave, F. Menard, W. R. F. Dent +13

Context. Characterizing the evolution of protoplanetary disks is necessary to improve our understanding of planet formation. Constraints on both dust and gas are needed to determin…

astro-ph.EP2021

Perturbers: SPHERE detection limits to planetary-mass companions in protoplanetary disks

R. Asensio-Torres, Th. Henning, F. Cantalloube +25

The detection of a wide range of substructures such as rings, cavities and spirals has become a common outcome of high spatial resolution imaging of protoplanetary disks, both in t…

astro-ph.SR2021

The Anatomy of an Unusual Edge-on Protoplanetary Disk. II. Gas temperature and a warm outer region

Christian Flores, Gaspard Duchene, Schuyler Wolff +9

We present high-resolution CO and CO 2-1 ALMA observations, as well as optical and near-infrared spectroscopy, of the highly-inclined protoplanetary disk around SSTC2…

astro-ph.SR2021

The Anatomy of an Unusual Edge-on Protoplanetary Disk I. Dust Settling in a Cold Disk

S. Wolff, G. Duchêne, K. Stapelfeldt +7

As the earliest stage of planet formation, massive, optically thick, and gas rich protoplanetary disks provide key insights into the physics of star and planet formation. When view…