collaborators

21 papers

astro-ph.SR2026

Far-ultraviolet flux distribution in Orion and its relation to stellar accretion

Rossella Anania, Andrew J. Winter, Miguel Vioque +8

Orion is the closest region hosting active star formation and young OBA stars. Computing far-ultraviolet (FUV) fluxes at its stars is essential to connect stellar and protoplanetar…

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 +20

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.EP2026

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): Constraints on disk turbulence, fragmentation velocity, and inner pebble fluxes

Lilian Luo, Paola Pinilla, Camila Pulgarés +14

How substructures and disk properties affect dust evolution and the delivery of solids and volatiles into planet-forming regions remains an open question. We present results from t…

astro-ph.EP2026

Survival of Protoplanetary Disks in Upper Scorpius from Population Synthesis Models with External Photoevaporation

Jingyi Ping, Rossella Anania, Paola Pinilla +1

We present population synthesis models of viscous protoplanetary disks subject to mild external far-ultraviolet (FUV) radiation fields (G). Our simul…

astro-ph.EP2026

A tension between dust and gas radii: the role of substructures and external photoevaporation in protoplanetary disks

Luca Delussu, Rossella Anania, Tilman Birnstiel +5

Protoplanetary disk substructures are thought to play a crucial role in disk evolution and planet formation. Population studies of disks large-sample size surveys show that substru…

astro-ph.EP2026

Timescales diagnostics for saving viscous and MHD-driven dusty discs from external photoevaporation

Gabriele Pichierri, Giovanni Rosotti, Rossella Anania +1

The evolution of protoplanetary discs is a function of their internal processes and of their environment. It is unclear if angular momentum is mainly removed viscously or by magnet…