Flybys in protoplanetary discs - II. Observational signatures

Nicolás Cuello; Fabien Louvet; Daniel Mentiplay; Christophe Pinte; Daniel J. Price; Andrew J. Winter; Rebecca Nealon; François Ménard; Giuseppe Lodato; Giovanni Dipierro; Valentin Christiaens; Matías Montesinos; Jorge Cuadra; Guillaume Laibe; Lucas Cieza; Ruobing Dong; Richard Alexander

doi:10.1093/mnras/stz2938

Flybys in protoplanetary discs - II. Observational signatures

Nicolás Cuello, Fabien Louvet, Daniel Mentiplay, Christophe Pinte, Daniel J. Price, Andrew J. Winter, Rebecca Nealon, François Ménard, Giuseppe Lodato, Giovanni Dipierro, Valentin Christiaens, Matías Montesinos, Jorge Cuadra, Guillaume Laibe, Lucas Cieza, Ruobing Dong, Richard Alexander

School of Physics and Astronomy

Research output: Contribution to journal › Article › Research › peer-review

59 Citations (Scopus)

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).

Original language	English
Pages (from-to)	504-514
Number of pages	11
Journal	Monthly Notices of the Royal Astronomical Society
Volume	491
Issue number	1
DOIs	https://doi.org/10.1093/mnras/stz2938
Publication status	Published - 1 Jan 2020

Keywords

Hydrodynamics
Methods: numerical
Planets and satellites: formation
Protoplanetary discs

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10.1093/mnras/stz2938

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Cuello, N., Louvet, F., Mentiplay, D., Pinte, C., Price, D. J., Winter, A. J., Nealon, R., Ménard, F., Lodato, G., Dipierro, G., Christiaens, V., Montesinos, M., Cuadra, J., Laibe, G., Cieza, L., Dong, R., & Alexander, R. (2020). Flybys in protoplanetary discs - II. Observational signatures. Monthly Notices of the Royal Astronomical Society, 491(1), 504-514. https://doi.org/10.1093/mnras/stz2938

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title = "Flybys in protoplanetary discs - II. Observational signatures",

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).",

keywords = "Hydrodynamics, Methods: numerical, Planets and satellites: formation, Protoplanetary discs",

author = "Nicol{\'a}s Cuello and Fabien Louvet and Daniel Mentiplay and Christophe Pinte and Price, {Daniel J.} and Winter, {Andrew J.} and Rebecca Nealon and Fran{\c c}ois M{\'e}nard and Giuseppe Lodato and Giovanni Dipierro and Valentin Christiaens and Mat{\'i}as Montesinos and Jorge Cuadra and Guillaume Laibe and Lucas Cieza and Ruobing Dong and Richard Alexander",

year = "2020",

month = jan,

day = "1",

doi = "10.1093/mnras/stz2938",

language = "English",

volume = "491",

pages = "504--514",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

}

Cuello, N, Louvet, F, Mentiplay, D, Pinte, C, Price, DJ, Winter, AJ, Nealon, R, Ménard, F, Lodato, G, Dipierro, G, Christiaens, V, Montesinos, M, Cuadra, J, Laibe, G, Cieza, L, Dong, R & Alexander, R 2020, 'Flybys in protoplanetary discs - II. Observational signatures', Monthly Notices of the Royal Astronomical Society, vol. 491, no. 1, pp. 504-514. https://doi.org/10.1093/mnras/stz2938

TY - JOUR

T1 - Flybys in protoplanetary discs - II. Observational signatures

AU - Cuello, Nicolás

AU - Louvet, Fabien

AU - Mentiplay, Daniel

AU - Pinte, Christophe

AU - Price, Daniel J.

AU - Winter, Andrew J.

AU - Nealon, Rebecca

AU - Ménard, François

AU - Lodato, Giuseppe

AU - Dipierro, Giovanni

AU - Christiaens, Valentin

AU - Montesinos, Matías

AU - Cuadra, Jorge

AU - Laibe, Guillaume

AU - Cieza, Lucas

AU - Dong, Ruobing

AU - Alexander, Richard

PY - 2020/1/1

Y1 - 2020/1/1

N2 - 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).

AB - 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).

KW - Hydrodynamics

KW - Methods: numerical

KW - Planets and satellites: formation

KW - Protoplanetary discs

UR - http://www.scopus.com/inward/record.url?scp=85079627971&partnerID=8YFLogxK

U2 - 10.1093/mnras/stz2938

DO - 10.1093/mnras/stz2938

M3 - Article

AN - SCOPUS:85079627971

SN - 0035-8711

VL - 491

SP - 504

EP - 514

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

Flybys in protoplanetary discs - II. Observational signatures

Abstract

Keywords

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Gaps, rings and holes in protoplanetary discs - signs of newborn planets?

Formation and evolution of planetary systems

The birth of stars and planets

Cite this

Flybys in protoplanetary discs - II. Observational signatures

Abstract

Keywords

Access to Document

Other files and links

Projects

Gaps, rings and holes in protoplanetary discs - signs of newborn planets?

Formation and evolution of planetary systems

The birth of stars and planets

Cite this