Evolution and Dispersal of Protoplanetary Disks

被引：0
|
作者：
Sicilia-Aguilar, A. [1 ]
Henning, Th. [1 ]
Juhasz, A. [1 ]
Bouwman, J. [1 ]
Hartmann, L. [2 ]
Watson, D. [3 ]
机构：
[1] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
[2] Univ Michigan, Ann Arbor, MI 48109 USA
[3] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA
来源：
COOL STARS, STELLAR SYSTEMS AND THE SUN | 2009年 / 1094卷
关键词：
Stars: Formation; Planetary systems: Protoplanetary disks; Accretion disks; INTERSTELLAR SILICATE MINERALOGY; ACCRETION; DUST; PLANET; PHOTOEVAPORATION; GROWTH; GRAINS; DISCS; STEPS; GAS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Multiwavelength studies of evolved protoplanetary disks around solar-type and low-mass stars reveal a general trend of changes in the IR excesses, accretion rates, and silicate features, suggesting grain growth/settling, photoevaporation, and maybe the formation of planetesimals and planets. Nevertheless within the average-behavior picture of disk evolution, we observe strong variations between individuals, that may be related to different initial conditions, different environments, and the presence of companions.
引用
收藏
页码：23 / +
页数：2
相关论文
共 50 条
  • [31] DUST EVOLUTION CAN PRODUCE SCATTERED LIGHT GAPS IN PROTOPLANETARY DISKS
    Birnstiel, Tilman
    Andrews, Sean M.
    Pinilla, Paola
    Kama, Mihkel
    ASTROPHYSICAL JOURNAL LETTERS, 2015, 813 (01)
  • [32] A SEMI-ANALYTICAL DESCRIPTION FOR THE FORMATION AND GRAVITATIONAL EVOLUTION OF PROTOPLANETARY DISKS
    Takahashi, Sanemichi Z.
    Inutsuka, Shu-ichiro
    Machida, Masahiro N.
    ASTROPHYSICAL JOURNAL, 2013, 770 (01):
  • [33] Evolution of protoplanetary disks: constraints from DM Tauri and GM Aurigae
    Hueso, R
    Guillot, T
    ASTRONOMY & ASTROPHYSICS, 2005, 442 (02) : 703 - 725
  • [34] The Time Evolution of Md/M? in Protoplanetary Disks as a Way to Disentangle between Viscosity and MHD Winds
    Somigliana, Alice
    Testi, Leonardo
    Rosotti, Giovanni
    Toci, Claudia
    Lodato, Giuseppe
    Tabone, Benoit
    Manara, Carlo F.
    Tazzari, Marco
    ASTROPHYSICAL JOURNAL LETTERS, 2023, 954 (01)
  • [35] Dust coagulation in protoplanetary disks: porosity matters
    Ormel, C. W.
    Spaans, M.
    Tielens, A. G. G. M.
    ASTRONOMY & ASTROPHYSICS, 2007, 461 (01) : 215 - 232
  • [36] From birth to death of protoplanetary discs: modelling their formation, evolution and dispersal
    Kimura, Shigeo S.
    Kunitomo, Masanobu
    Takahashi, Sanemichi Z.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 461 (02) : 2257 - 2265
  • [37] ROTATIONAL INSTABILITY IN THE OUTER REGION OF PROTOPLANETARY DISKS
    Ono, Tomohiro
    Nomura, Hideko
    Takeuchi, Taku
    ASTROPHYSICAL JOURNAL, 2014, 787 (01):
  • [38] A simple model for the evolution of the dust population in protoplanetary disks
    Birnstiel, T.
    Klahr, H.
    Ercolano, B.
    ASTRONOMY & ASTROPHYSICS, 2012, 539
  • [39] Global evolution of solids in protoplanetary disks:: A simple model
    Rózyczka, M
    Kornet, K
    Bodenheimer, P
    Stepinski, T
    GRAVITATIONAL COLLAPSE: FROM MASSIVE STARS TO PLANETS, 2004, 22 : 91 - 94
  • [40] EFFECTS OF DUST FEEDBACK ON VORTICES IN PROTOPLANETARY DISKS
    Fu, Wen
    Li, Hui
    Lubow, Stephen
    Li, Shengtai
    Liang, Edison
    ASTROPHYSICAL JOURNAL LETTERS, 2014, 795 (02)
12345