Flybys in protoplanetary discs - II. Observational signatures

被引:59
作者
Cuello, Nicolas [1 ,2 ,3 ]
Louvet, Fabien [4 ]
Mentiplay, Daniel [5 ,6 ]
Pinte, Christophe [5 ,6 ,7 ]
Price, Daniel J. [5 ,6 ]
Winter, Andrew J. [3 ]
Nealon, Rebecca [3 ]
Menard, Francois [7 ]
Lodato, Giuseppe [8 ]
Dipierro, Giovanni [3 ]
Christiaens, Valentin [5 ,6 ]
Montesinos, Matias [2 ,9 ,10 ]
Cuadra, Jorge [1 ,2 ]
Laibe, Guillaume [11 ]
Cieza, Lucas [12 ]
Dong, Ruobing [13 ]
Alexander, Richard [3 ]
机构
[1] Pontificia Univ Catolica Chile, Inst Astrofis, Santiago, Chile
[2] Nucleo Milenio Formac Planetaria NPF, Valparaiso, Chile
[3] Univ Leicester, Sch Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, England
[4] Univ Chile, Dept Astron Chile, Santiago, Chile
[5] Monash Univ, Monash Ctr Astrophys MoCA, Clayton, Vic 3800, Australia
[6] Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
[7] Univ Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France
[8] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy
[9] Univ Valparaiso, Fac Ciencias, Inst Fis & Astron, Valparaiso 1111, Chile
[10] Chinese Acad Sci, South Amer Ctr Astron, Natl Astron Observ, Beijing 100012, Peoples R China
[11] Univ Lyon 1, Univ Lyon, Ens Lyon, CNRS,Ctr Rech Astrophys Lyon,UMR5574, F-69230 St Genis Laval, France
[12] Univ Diego Portales, Nucleo Astron, Fac Ingn & Ciencias, Av Ejercito 441, Santiago, Chile
[13] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 1A1, Canada
基金
欧洲研究理事会; 澳大利亚研究理事会; 欧盟地平线“2020”;
关键词
hydrodynamics; methods: numerical; planets and satellites: formation; protoplanetary discs; EXTERNAL PHOTOEVAPORATION; CIRCUMSTELLAR DISKS; CIRCUMBINARY DISCS; RADIATIVE-TRANSFER; WARP PROPAGATION; SPIRAL ARMS; MASS-LOSS; ACCRETION; DUST; I;
D O I
10.1093/mnras/stz2938
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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).
引用
收藏
页码:504 / 514
页数:11
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