activity
20182026
most citedFlybys in protoplanetary discs: I. Gas and dust dynamics

142 citations · 809 across the 32 of their papers we have counts for

collaborators

34 papers

astro-ph.IM2026

Planet forming disk populations and their connection to the environment

Thomas J. Haworth, Giovanni Rosotti, Carlo Manara +35

Existing sub-mm observatories such as ALMA have provided statistics on the planet-forming mass reservoirs within circumstellar disks around stars in stellar clusters out to distanc…

astro-ph.EP2026

Binary tidal evolution as a sculptor of circumbinary planet architectures

Mario Sucerquia, Nicolás Cuello, Gaspard Duchêne

Circumbinary planets (CBPs) are expected to form in circumbinary discs and migrate towards the disc inner cavity, often near the binary stability boundary. Yet the observed populat…

astro-ph.SR2026

ALMA's sharpest view of IRAS 08544-4431: Unveiling the dust distribution asymmetries in the circumbinary disk

Maksym Mohorian, Devika Kamath, Elizabeth Cappellazzo +10

The interactions between post-asymptotic giant branch (post-AGB) binaries and their circumbinary disks play a central role in shaping the evolution of these systems. Circumbinary d…

astro-ph.EP2026

Stability of circumbinary planets: the role of binary properties and migration scenarios

Romain Grane, Nicolás Cuello, Mario Sucerquia +4

Among the thousands of exoplanets detected to date, only a very small fraction are classified as circumbinary planets, and this number becomes negligible when considering low-mass…

astro-ph.EP2026

Circumbinary planets in coplanar triple-star systems: I. Minimum eccentricity variation region

Emmanuel Gianuzzi, Mario Sucerquia, Nicolás Cuello +1

We aim to determine the conditions under which Lidov-Kozai oscillations can arise for circumbinary planets in hierarchical triple-star systems, and to identify the orbital regions…

astro-ph.EP2026

Dust Growth in Binary Systems: Inhibition of dust settling and growth in circumbinary discs

Antoine Alaguero, Nicolás Cuello, Jean-François Gonzalez +4

Stellar multiplicity alters the density structure of protoplanetary discs and thereby the initial conditions for planet formation. Yet, the interplay between companion-disc interac…