activity
20022026
most citedThe size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

258 citations · 4.8k across the 110 of their papers we have counts for

collaborators

111 papers

astro-ph.EP2026

Dust torques for realistic dust size distributions

V. Roatti, G. Picogna, F. Marzari

Previous studies have shown that a population of dust particles with a fixed Stokes number can exert a substantial torque on a low-mass planet embedded in a protoplanetary disk, mo…

astro-ph.EP2024

Long term dynamics around the Didymos-Dimorphos binary asteroid of boulders ejected after the DART impact

Krzysztof Langner, Francesco Marzari, Alessandro Rossi +1

In 2022 the DART mission spacecraft impacted the asteroid Dimorphos, the secondary body of the binary Didymos system, ejecting a large number of dust particles, rocks and boulders.…

astro-ph.EP2023★ 18 cited

The GAPS program at TNG XLVII: The unusual formation history of V1298 Tau

D. Turrini, F. Marzari, D. Polychroni +33

Observational data from space and ground-based campaigns reveal that the 10-30 Ma old V1298 Tau star hosts a compact and massive system of four planets. Mass estimates for the two…

astro-ph.EP2023★ 22 cited

The GAPS Programme at TNG XLII. A characterisation study of the multi-planet system around the 400 Myr-old star HD 63433 (TOI-1726)

M. Damasso, D. Locci, S. Benatti +34

For more than two years, we monitored with the HARPS-N spectrograph the 400 Myr-old star HD\,63433, which hosts two close-in (orbital periods and days) s…

astro-ph.EP2023★ 1 cited

Effects of turbulent diffusion and back-reaction on the dust distribution around two resonant planets

Francesco Marzari, Gennaro DAngelo

In evolved and dusty circumstellar discs, two planets with masses comparable to Jupiter and Saturn that migrate outwards while maintaining an orbital resonance can produce distinct…

astro-ph.SR2022★ 1 cited

The SPHERE view of multiple star formation

R. Gratton, S. Desidera, F. Marzari +1

While a large fraction of the stars are in multiple systems, our understanding of the processes leading to the formation of these systems is still inadequate. Given the large theor…