Flybys in protoplanetary discs – II. Observational signatures

Tidal encounters in star clusters perturb discs around young protostars. In Cuello et al., we detailed the dynamical signatures of a stellar flyby in both gas and dust. Flybys produce warped discs, spirals with evolving pitch angles, increasing accretion rates, and disc truncation. Here, we present...

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Bibliographic Details
Published in:	Monthly notices of the Royal Astronomical Society Vol. 491; no. 1; pp. 504 - 514
Main Authors:	Cuello, Nicolás, Louvet, Fabien, Mentiplay, Daniel, Pinte, Christophe, Price, Daniel J, Winter, Andrew J, Nealon, Rebecca, Ménard, François, Lodato, Giuseppe, Dipierro, Giovanni, Christiaens, Valentin, Montesinos, Matías, Cuadra, Jorge, Laibe, Guillaume, Cieza, Lucas, Dong, Ruobing, Alexander, Richard
Format:	Journal Article
Language:	English
Published:	Oxford University Press (OUP): Policy P - Oxford Open Option A 01.01.2020 Oxford University Press
Subjects:	Astrophysics - Astrophysics of Galaxies Astrophysics - Earth and Planetary Astrophysics Astrophysics - Solar and Aérospatiale, astronomie & astrophysique hydrodynamics methods: numerical Physical, chemical, mathematical & earth Sciences Physique, chimie, mathématiques & sciences de la terre planets and satellites: formation protoplanetary discs Sciences of the Universe Space science, astronomy & astrophysics Stellar Astrophysics Astrophysics - Astrophysics of Galaxies protoplanetary discs Astrophysics - Earth and Planetary Astrophysics hydrodynamics methods: numerical planets and satellites: formation Astrophysics - Solar and Stellar Astrophysics
ISSN:	0035-8711, 1365-2966, 1365-2966
Online Access:	Get full text
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