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
Showing 2022Show all

9 papers · 1 filter

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.EP2022★ 58 cited

Directly tracing the vertical stratification of molecules in protoplanetary disks

T. Paneque-Carreño, A. Miotello, E. F. van Dishoeck +3

We aim to directly trace the vertical location of the emitting surface of multiple molecular tracers in protoplanetary disks. Our sample of disks includes Elias 2-27, WaOph 6 and t…

astro-ph.IM2022

The Present and Future of Astronomy (ASTRO2022)

Giacomo Beccari, Henri M. J. Boffin, Paola Andreani +7

Being one of the most fascinating and ancient sciences, astronomy has always played a special role in society. In 2022 ESO organised an online conference to offer the community a p…

astro-ph.EP2022★ 18 cited

Vertically extended and asymmetric CN emission in the Elias 2-27 protoplanetary disk

T. Paneque-Carreño, A. Miotello, E. F. van Dishoeck +5

Elias 2-27 is a young star that hosts an extended, bright and inclined disk of dust and gas. The inclination and extreme flaring of the disk make Elias 2-27 an ideal target to stud…

astro-ph.GA2022★ 22 cited

Hot methanol in the [BHB2007] 11 protobinary system: hot corino versus shock origin? : FAUST V

C. Vastel, F. Alves, C. Ceccarelli +63

Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the building-up of the chemical complexity in star formi…

astro-ph.SR2022★ 20 cited

Chemical and Physical Characterization of the Isolated Protostellar Source CB68: FAUST. IV

Muneaki Imai, Yoko Oya, Brian Svoboda +1

Chemical diversity of low-mass protostellar sources has so far been recognized, and environmental effects are invoked as its origin. In this context, observations of isolated proto…