activity
20162026
most citedALMA observations of the early stages of substellar formation in the Lupus 1 and 3 molecular clouds

10 citations · 26 across the 6 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2025

Hints of Disk Substructure in the First Brown Dwarf with a Dynamical Mass Constraint

Alejandro Santamaría Miranda, Pietro Curone, Laura Pérez +14

We present high-resolution ALMA observations at 0.89 mm of the Class II brown dwarf 2MASS J04442713+2512164 (2M0444), achieving a spatial resolution of 0046 (…

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.SR2020★ 9 cited

Bipolar molecular outflow of the very low-mass star Par-Lup3-4

A. Santamaría-Miranda, I. de Gregorio-Monsalvo, N. Huélamo +7

Very low-mass stars are known to have jets and outflows, which is indicative of a scaled-down version of low-mass star formation. However, only very few outflows in very low-mass s…

astro-ph.SR2019

Dust production in the debris disk around HR 4796 A

J. Olofsson, J. Milli, P. Thébault +21

Debris disks are the natural by-products of the planet formation process. Scattered or polarized light observations are mostly sensitive to small dust grains that are released from…

astro-ph.SR2018

Alma Survey Of Circumstellar Disks In The Young Stellar Cluster IC 348

D. Ruíz-Rodríguez, L. A. Cieza, J. P. Williams +7

We present a 1.3 mm continuum survey of the young (2-3 Myr) stellar cluster IC 348, which lies at a distance of 310 pc, and is dominated by low-mass stars (M 0.1-0…

astro-ph.SR2016

Constraining the mass of the planet(s) sculpting a disk cavity. The intriguing case of 2MASS J16042165-2130284

H. Canovas, A. Hardy, A. Zurlo +10

The large cavities observed in the dust and gas distributions of transition disks may be explained by planet-disk interactions. At ~145 pc, 2MASS J16042165-2130284 (J1604) is a 5-1…