A simple criterion for selecting disks with evidence for dust growth and settling

被引:0
|
作者
Yao Liu
Hongchi Wang
Thomas Henning
机构
[1] Chinese Academy of Sciences,Purple Mountain Observatory & Key Laboratory for Radio Astronomy
[2] Max Planck Institute for Astronomy,undefined
来源
关键词
Circumstellar matter; Planetary systems: protoplanetary disks; Radiative transfer;
D O I
暂无
中图分类号
学科分类号
摘要
Dust growth and settling, as an initial step of planet formation in protoplanetary disks, have an important impact on the appearance of the spectral energy distribution (SED). Selecting a promising sample of disks with signs of these processes helps to guide future observations towards a better understanding of the initial conditions for planet formation and disk evolution. Using a standard flared disk model, we conducted a large parameter study to investigate the effects of various disk parameters on the overall shape of the SED. We found that the flaring index and scale height can be used to mimic the effects of dust evolution on the SED. The influences of these two parameters on the infrared excess are very similar to that caused by dust evolution which have been shown in previous simulations where grain growth and settling are treated directly. Based on a statistic analysis of all the models in our grid, we proposed a criterion of Ψ≥0.6\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\varPsi \ge 0.6$\end{document} to diagnose signs of dust evolution, where Ψ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\varPsi$\end{document} is a ratio defined by dividing a linearly interpolated (between 24μm\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$24~\upmu \mbox{m}$\end{document} and 1.3 mm) flux at 70 μm by the observed 70 μm photometry. We tested the applicability of our criterion with the class II disks in the Taurus star formation region.
引用
收藏
相关论文
共 50 条
  • [1] A simple criterion for selecting disks with evidence for dust growth and settling
    Liu, Yao
    Wang, Hongchi
    Henning, Thomas
    ASTROPHYSICS AND SPACE SCIENCE, 2017, 362 (11)
  • [2] Growth of Settling Dust Particles in Turbulent Disks
    Takeuchi, Taku
    EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY, 2009, 1158 : 163 - 164
  • [3] Effects of dust growth and settling in T Tauri disks
    D'Alessio, P
    Calvet, N
    Hartmann, L
    Franco-Hernández, R
    Servín, H
    ASTROPHYSICAL JOURNAL, 2006, 638 (01): : 314 - 335
  • [4] DoAr 33: a good candidate for revealing dust growth and settling in protoplanetary disks
    Liu, Y.
    Madlener, D.
    Wolf, S.
    Wang, H.
    Ruge, J. Philipp
    ASTRONOMY & ASTROPHYSICS, 2012, 546
  • [5] The effect of dust settling on the appearance of protoplanetary disks
    Dullemond, C.P.
    Dominik, C.
    Astronomy and Astrophysics, 1600, 421 (03): : 1075 - 1086
  • [6] Dust coagulation and settling in layered protoplanetary disks
    Ciesla, Fred J.
    ASTROPHYSICAL JOURNAL, 2007, 654 (02): : L159 - L162
  • [7] The effect of dust settling on the appearance of protoplanetary disks
    Dullemond, CP
    Dominik, C
    ASTRONOMY & ASTROPHYSICS, 2004, 421 (03) : 1075 - 1086
  • [8] Evidence for dust grain growth in young circumstellar disks
    Throop, HB
    Bally, J
    Esposito, LW
    McCaughrean, MJ
    SCIENCE, 2001, 292 (5522) : 1686 - 1689
  • [9] Dust growth and settling in protoplanetary disks and disk spectral energy distributions. I. Laminar disks
    Tanaka, H
    Himeno, Y
    Ida, S
    ASTROPHYSICAL JOURNAL, 2005, 625 (01): : 414 - 426
  • [10] Dust settling and dust processing in protoplanetary disks around cool stars
    Apai, D.
    Pascucci, I.
    METEORITICS & PLANETARY SCIENCE, 2007, 42 : A14 - A14