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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Vydáno v:Monthly notices of the Royal Astronomical Society Ročník 491; číslo 1; s. 504 - 514
Hlavní autoři: 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
Médium: Journal Article
Jazyk:angličtina
Vydáno: Oxford University Press (OUP): Policy P - Oxford Open Option A 01.01.2020
Oxford University Press
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ISSN:0035-8711, 1365-2966, 1365-2966
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Abstract 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 the corresponding observational signatures of these features in optical/near-infrared scattered light and (sub) millimetre continuum and CO line emission. Using representative prograde and retrograde encounters for direct comparison, we post-process hydrodynamical simulations with radiative transfer methods to generate a catalogue of multiwavelength observations. This provides a reference to identify flybys in recent near-infrared and submillimetre observations (e.g. RW Aur, AS 205, HV Tau and DO Tau, FU Ori, V2775 Ori, and Z CMa).
AbstractList 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 the corresponding observational signatures of these features in optical/near-infrared scattered light and (sub) millimetre continuum and CO line emission. Using representative prograde and retrograde encounters for direct comparison, we post-process hydrodynamical simulations with radiative transfer methods to generate a catalogue of multiwavelength observations. This provides a reference to identify flybys in recent near-infrared and submillimetre observations (e.g. RW Aur, AS 205, HV Tau and DO Tau, FU Ori, V2775 Ori, and Z CMa).
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 the corresponding observational signatures of these features in optical/near-infrared scattered light and (sub) millimetre continuum and CO line emission. Using representative prograde and retrograde encounters for direct comparison, we post-process hydrodynamical simulations with radiative transfer methods to generate a catalogue of multiwavelength observations. This provides a reference to identify flybys in recent near-infrared and submillimetre observations (e.g. RW Aur, AS 205, HV Tau and DO Tau, FU Ori, V2775 Ori, and Z CMa).
Author Price, Daniel J
Cuadra, Jorge
Alexander, Richard
Louvet, Fabien
Cuello, Nicolás
Nealon, Rebecca
Mentiplay, Daniel
Dong, Ruobing
Dipierro, Giovanni
Lodato, Giuseppe
Christiaens, Valentin
Cieza, Lucas
Montesinos, Matías
Pinte, Christophe
Ménard, François
Winter, Andrew J
Laibe, Guillaume
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  organization: Univ. Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France
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  orcidid: 0000-0002-2357-7692
  surname: Lodato
  fullname: Lodato, Giuseppe
  organization: Dipartimento di Fisica, Università Degli Studi di Milano, Via Celoria, 16, I-20133 Milano, Italy
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  orcidid: 0000-0002-7185-5458
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  organization: School of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK
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  surname: Montesinos
  fullname: Montesinos, Matías
  organization: Núcleo Milenio de Formación Planetaria (NPF), Chile, Inst. Física y Astronomía, Fac. Ciencias, Universidad de Valparaíso, Gran Bretaña 1111, Valparaíso, Chile, Chinese Academy of Sciences South America Center for Astronomy, National Astronomical Observatories, CAS, Beijing 100012, China
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  organization: Instituto de Astrofísica, Pontificia Universidad Católica de Chile, Santiago, Chile, Núcleo Milenio de Formación Planetaria (NPF), Chile
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  organization: Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, F-69230 Saint-Genis-Laval, France
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  surname: Cieza
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  organization: Facultad de Ingeniería y Ciencias, Núcleo de Astronomía, Universidad Diego Portales, Av. Ejercito 441, Santiago, Chile
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  surname: Dong
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  organization: Department of Physics & Astronomy, University of Victoria, Victoria, BC V8P 1A1, Canada
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  givenname: Richard
  orcidid: 0000-0001-6410-2899
  surname: Alexander
  fullname: Alexander, Richard
  organization: Univ. Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France
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ISSN 0035-8711
1365-2966
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Issue 1
Keywords Astrophysics - Astrophysics of Galaxies
protoplanetary discs
Astrophysics - Earth and Planetary Astrophysics
hydrodynamics
methods: numerical
planets and satellites: formation
Astrophysics - Solar and Stellar Astrophysics
Language English
License https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model
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Publisher Oxford University Press (OUP): Policy P - Oxford Open Option A
Oxford University Press
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Snippet 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...
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...
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SubjectTerms 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
Title Flybys in protoplanetary discs – II. Observational signatures
URI https://insu.hal.science/insu-03705227
https://orbi.uliege.be/handle/2268/310960
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