activity
20102024
most citedShadows cast by a warp in the HD 142527 protoplanetary disk

256 citations · 904 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.EP20243 cited

Polarimetric differential imaging with VLT/NACO. A comprehensive PDI pipeline for NACO data (PIPPIN)

S. de Regt, C. Ginski, M. A. Kenworthy +9

The observed diversity of exoplanets can possibly be traced back to the planet formation processes. Planet-disk interactions induce sub-structures in the circumstellar disk that ca…

astro-ph.SR2024

The environment around young eruptive stars. SPHERE/IRDIS polarimetric imaging of 7 protostars

A. Zurlo, P. Weber, S. Pérez +11

Eruptive stars are a class of young stellar objects that show an abrupt increase in their luminosity. These burst-like episodes are thought to dominate the stellar accretion proces…

astro-ph.GA2024

The SPHERE view of the Taurus star-forming region

A. Garufi, C. Ginski, R. G. van Holstein +31

The sample of planet-forming disks observed by high-contrast imaging campaigns over the last decade is mature enough to enable the demographical analysis of individual star-forming…

astro-ph.EP2023

Radio-continuum decrements associated to shadowing from the central warp in transition disc DoAr44

Carla Arce-Tord, Simon Casassus, William R. F. Dent +8

Warps have often been used to explain disc properties, but well characterised examples are important due to their role in disc evolution. Scattered light images of discs with centr…

astro-ph.EP202317 cited

Spirals and clumps in V960 Mon: signs of planet formation via gravitational instability around an FU Ori star?

P. Weber, S. Pérez, A. Zurlo +11

The formation of giant planets has traditionally been divided into two pathways: core accretion and gravitational instability. However, in recent years, gravitational instability h…

astro-ph.EP202315 cited

Inner edges of planetesimal belts: collisionally eroded or truncated?

Amaia Imaz Blanco, Sebastian Marino, Luca Matrà +9

The radial structure of debris discs can encode important information about their dynamical and collisional history. In this paper we present a 3-phase analytical model to analyse…