activity
20122026
most citedALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses

617 citations · 5.1k across the 84 of their papers we have counts for

collaborators

83 papers

astro-ph.EP2026

A faint dust ring beyond the compact disk of Sz 76

Giulia Ricciardi, Anna Miotello, Karina Mauco +9

We report new ALMA Band 7 high-resolution (0.05) continuum and observations of the disk around the young low-mass star Sz 76. Visibil…

astro-ph.SR2026

FAUST XXXI. Grain properties and variability of three sources in GSS 30

Q. Yang, H. Baobab Liu, S. Feng +55

To advance our understanding of dust properties in class 0/I young stellar objects, it is crucial to resolve their structures at multiple wavelengths and investigate how grain grow…

astro-ph.SR2026

X-Shooter survey of disk accretion in Upper Scorpius II. A lack of correlation between accretion rates and disk properties

A. Empey, C. F. Manara, R. Garcia Lopez +19

The evolution of protoplanetary discs is intertwined with the process of planet formation, growth and migration. Studies of nearby star forming regions of different ages and proper…

astro-ph.GA2026★ 1 cited

The environmental imprint on molecular layering in the dusty streamer of M512

M. De Simone, L. Cacciapuoti, D. Capela +7

Protostellar streamers are elongated structures that channel material from larger scale onto disks, influencing their physical and chemical evolution. The M512 protostar in Orion/L…

astro-ph.EP2026★ 1 cited

Compact CO emission and no evidence of radial drift. ALMA observations of the faintest planet-forming disks in Lupus

Giulia Ricciardi, Francesco Zagaria, Anna Miotello +13

A large fraction of planet-forming disks observed with ALMA show faint CO emission, often interpreted as strong CO depletion. However, faint emission may also arise from spatially…

astro-ph.SR2026

Benchmarking pre-main sequence stellar evolutionary tracks using disk-based dynamical stellar masses

Luigi Zallio, Miguel Vioque, Sean M. Andrews +14

Stellar masses are a fundamental property to understand models of pre-main sequence evolution, but their values derived from Hertzsprung-Russell (HR) diagrams are strongly model de…