most citedDust unveils the formation of a mini-Neptune planet in a protoplanetary ring

105 citations · 334 across the 10 of their papers we have counts for

collaborators

14 papers

astro-ph.SR202017 cited

ALMA Observations of Young Eruptive Stars: continuum disk sizes and molecular outflows

Antonio S. Hales, Sebastián Pérez, Camilo Gonzalez-Ruilova +7

We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm observations of four young, eruptive star-disk systems at 0.4" resolution: two FUors (V582 Aur and V900 Mon),…

physics.pop-ph2020

The Artscience of Planet Formation: import ArtScience.PlanetFormation as AATS

Sebastián Pérez

The Art, Astronomy, Technology and Society (AATS) project is an artscience collaboration which dwells in the inbetweenness layer of scientific understanding of the origins of plane…

astro-ph.SR20198 cited

SUBARU Near-Infrared Imaging Polarimetry of Misaligned Disks Around The SR24 Hierarchical Triple System

Satoshi Mayama, Sebastián Pérez, Nobuhiko Kusakabe +65

The SR24 multi-star system hosts both circumprimary and circumsecondary disks, which are strongly misaligned from each other. The circumsecondary disk is circumbinary in nature. In…

astro-ph.EP201956 cited

Resolving the FU Ori System with ALMA: Interacting Twin Disks?

Sebastián Pérez, Antonio Hales, Hauyu Baobab Liu +7

FU Orionis objects are low-mass pre-main sequence stars characterized by dramatic outbursts of several magnitudes in brightness. These outbursts are linked to episodic accretion ev…

astro-ph.EP201953 cited

Predicting the observational signature of migrating Neptune-sized planets in low-viscosity disks

Philipp Weber, Sebastián Pérez, Pablo Benítez-Llambay +3

The migration of planetary cores embedded in a protoplanetary disk is an important mechanism within planet-formation theory, relevant for the architecture of planetary systems. Con…

astro-ph.SR2019

Diagnosing 0.1-10 au scale morphology of the FU\,Ori disk using ALMA and VLTI/GRAVITY

Hauyu Baobab Liu, Antoine Mérand, Joel D. Green +11

We report new Atacama Large Millimeter/submillimeter Array Band 3 (86-100 GHz; 80 mas angular resolution) and Band 4 (146-160 GHz; 50 mas angular resolution) observatio…