activity
20232025
most citedConfirmation of a ring structure in the disk around MP Mus (PDS 66) with ALMA Band 7 observations

4 citations · 8 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025★ 4 cited

Confirmation of a ring structure in the disk around MP Mus (PDS 66) with ALMA Band 7 observations

Aurora Aguayo, Claudio Caceres, Zhen Guo +10

Young stellar objects (YSOs) are surrounded by protoplanetary disks, which are the birthplace of young planets. Ring and gap structures are observed among evolved protoplanetary di…

astro-ph.EP2025

A Multi-Wavelength Study of the Dynamic Environment surrounding the FUor V960 Mon

Philipp Weber, Silvio Ulloa, Sebastián Pérez +11

The evolution of young stars and planet-forming environments is intrinsically linked to their nascent surroundings. This is particularly evident for FU Orionis (FUor) objectsa c…

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.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.SR2023

Viscous heating as the dominant heat source inside the water snowline of V883 Ori

Felipe Alarcón, Simón Casassus, Wladimir lyra +2

FU Orionis-type objects(FUors) are embedded protostars that undergo episodes of high accretion, potentially indicating a widespread but poorly understood phase in the formation of…