activity
20152025
most citedSpiral Arms and a Massive Dust Disk with non-Keplerian Kinematics: Possible Evidence for Gravitational Instability in the Disk of Elias 2-27

75 citations · 489 across the 13 of their papers we have counts for

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11 papers · 1 filter

astro-ph.EP2025★ 24 cited

Mapping the merging zone of late infall in the AB Aur planet-forming system

Jessica Speedie, Ruobing Dong, Richard Teague +10

Late infall events challenge the traditional view that planet formation occurs without external influence. Here we present deep ALMA CO and SO observ…

astro-ph.EP2024★ 51 cited

Gravitational instability in a planet-forming disk

Jessica Speedie, Ruobing Dong, Cassandra Hall +7

The canonical theory for planet formation in circumstellar disks proposes that planets are grown from initially much smaller seeds. The long-considered alternative theory proposes…

astro-ph.EP2024★ 10 cited

Weighing protoplanetary discs with kinematics: physical model, method and benchmark

Benedetta Veronesi, Cristiano Longarini, Giuseppe Lodato +4

The mass of protoplanetary discs sets the amount of material available for planet formation, determines the level of coupling between gas and dust, and possibly sets gravitational…

astro-ph.EP2022★ 52 cited

Dynamical mass measurements of two protoplanetary discs

G. Lodato, L. Rampinelli, E. Viscardi +8

ALMA observations of line emission from planet forming discs have demonstrated to be an excellent tool to probe the internal disc kinematics, often revealing subtle effects related…

astro-ph.EP2021★ 25 cited

Investigating Protoplanetary Disk Cooling through Kinematics: Analytical GI Wiggle

Cristiano Longarini, Giuseppe Lodato, Claudia Toci +4

It is likely that young protostellar disks undergo a self-gravitating phase. Such systems are characterized by the presence of a spiral pattern that can be either in a quasi-steady…

astro-ph.EP2021★ 1 cited

Constraining protoplanetary disc mass using the GI wiggle

J. P. Terry, C. Hall, Cristiano Longarini +5

Exoplanets form in protoplanetary accretion discs. The total protoplanetary disc mass is the most fundamental parameter, since it sets the mass budget for planet formation. Althoug…

astro-ph.EP2021★ 60 cited

A dynamical measurement of the disk mass in Elias 2-27

Benedetta Veronesi, Teresa Paneque-Carreno, Giuseppe Lodato +4

Recent multi-wavelength ALMA observations of the protoplanetary disk orbiting around Elias 2-27 revealed a two armed spiral structure. The observed morphology together with the you…

astro-ph.EP2021★ 75 cited

Spiral Arms and a Massive Dust Disk with non-Keplerian Kinematics: Possible Evidence for Gravitational Instability in the Disk of Elias 2-27

T. Paneque-Carreño, L. M. Perez, M. Benisty +16

To determine the origin of the spiral structure observed in the dust continuum emission of Elias 2-27 we analyze multi-wavelength continuum ALMA data with a resolution of 0.2…

astro-ph.EP2020★ 21 cited

Is the gap in the DS Tau disc hiding a planet?

Benedetta Veronesi, Enrico Ragusa, Giuseppe Lodato +6

Recent mm-wavelength surveys performed with the Atacama Large Millimeter Array (ALMA) have revealed protoplanetary discs characterized by rings and gaps. A possible explanation for…

astro-ph.EP2019★ 20 cited

Multi-wavelength observations of protoplanetary discs as a proxy for the gas disc mass

B. Veronesi, G. Lodato, G. Dipierro +3

Recent observations of protoplanetary discs reveal disc substructures potentially caused by embedded planets. We investigate how the gas surface density in discs changes the observ…

astro-ph.EP2018★ 42 cited

Enforcing dust mass conservation in 3D simulations of tightly-coupled grains with the Phantom SPH code

Giulia Ballabio, Giovanni Dipierro, Benedetta Veronesi +4

We describe a new implementation of the one-fluid method in the SPH code Phantom to simulate the dynamics of dust grains in gas protoplanetary discs. We revise and extend previousl…