activity
20142026
most citedCircumbinary, not transitional: On the spiral arms, cavity, shadows, fast radial flows, streamers and horseshoe in the HD142527 disc

186 citations · 1.2k across the 75 of their papers we have counts for

collaborators
Showing 2022Show all

6 papers · 1 filter

astro-ph.SR2022★ 22 cited

The SPHERE view of three interacting twin disc systems in polarised light

Philipp Weber, Sebastián Pérez, Greta Guidi +12

Dense stellar environments as hosts of ongoing star formation increase the probability of gravitational encounters among stellar systems during the early stages of evolution. Stell…

astro-ph.EP2022★ 6 cited

Circumbinary planets: migration, trapping in mean-motion resonances, and ejection

Emmanuel Gianuzzi, Cristian A. Giuppone, Nicolás Cuello

Most of the planetary systems discovered around binary stars are located at approximately three semi-major axes from the barycentre of their system, curiously close to low-order me…

astro-ph.SR2022★ 29 cited

Sustained FU Orionis-type outbursts from colliding discs in stellar flybys

Elisabeth M. A. Borchert, Daniel J. Price, Christophe Pinte +1

We perform 3D hydrodynamics simulations of disc-disc stellar flybys with on-the-fly Monte Carlo radiative transfer. We show that pre-existing circumstellar discs around both stars…

astro-ph.EP2022★ 2 cited

Close encounters: How stellar flybys shape planet-forming discs

Nicolás Cuello, François Ménard, Daniel J. Price

We review the role of stellar flybys and encounters in shaping planet-forming discs around young stars, based on the published literature on this topic in the last 30 years. Since…

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

Accretion rates in hierarchical triple systems with discs

Simone Ceppi, Nicolás Cuello, Giuseppe Lodato +3

Young multiple systems accrete most of their final mass in the first few Myr of their lifetime, during the protostellar and protoplanetary phases. Previous studies showed that in b…