activity
20032026
most citedDust and Gas in the disc of HL Tauri: Surface density, dust settling, and dust-to-gas ratio

440 citations · 2.7k across the 63 of their papers we have counts for

collaborators

65 papers

astro-ph.IM2026

Bridging the gap between stars and planets

Aina Palau, Dimitris Stamatellos, Matthew Bate +58

The formation mechanisms of brown dwarfs (BDs) and free-floating planets (FFPs) are poorly constrained. The two main competing scenarios include the star-like scenario, where these…

astro-ph.SR2026

Complex morphology and kinematics at the heart of the very low luminosity object IRAM 04191+1522

N. Otten, I. de Gregorio-Monsalvo, N. Huélamo +3

The formation of the majority of brown dwarfs (BDs) remains uncertain. They may form in molecular cloud cores in a process akin to low mass star formation, or via fragmentation in…

astro-ph.EP2026

Two inner dust clumps in PDS 70. A third protoplanet traced by trojan material or a substructured inner disk?

O. Balsalobre-Ruza, V. Christiaens, N. Huélamo +18

The PDS 70 cavity hosts two confirmed directly imaged protoplanets and a third inner planet candidate at 13au, labeled PDS 70 d. Despite its Keplerian motion, its unusually blue sp…

astro-ph.GA2025★ 2 cited

Bowshocks driven by the pole-on molecular jet of outbursting protostar SVS 13

G. Blázquez-Calero, G. Anglada, S. Cabrit +13

Outflows play a key role in the star and planet formation processes. Some outflows show discrete clumps of cold molecular gas moving at extremely high velocities (EHVs) of 10…

astro-ph.SR2025

Early Planet Formation in Embedded Disks (eDisk). XIX. Structures of molecular outflows

Anton Feeney-Johansson, Yuri Aikawa, Shigehisa Takakuwa +13

As part of the ALMA Large Program "Early Planet Formation in Embedded Disks" (eDisk), 12CO (2 - 1) was observed towards 19 nearby low-mass protostars. Of these objects, 15 sources…

astro-ph.EP2025★ 11 cited

A young gas giant and hidden substructures in a protoplanetary disk

Álvaro Ribas, Miguel Vioque, Francesco Zagaria +7

The detection of planets in protoplanetary disks has proven to be extremely challenging. In contrast, rings and gaps, usually attributed to planet-disk interactions, have been foun…