Gas Evolution in Protoplanetary Disks

被引:0
|
作者
Woitke, Peter [1 ]
Dent, Bill [1 ]
Thi, Wing-Fai [1 ]
Sibthorpe, Bruce [1 ]
Rice, Ken [2 ]
Williams, Jonathan [3 ]
Sicilia-Aguilar, Aurora [4 ]
Brown, Joanna [5 ]
Kamp, Inga [6 ]
Pascucci, Ilaria [7 ]
Alexander, Richard [8 ]
Roberge, Aki [9 ]
机构
[1] Royal Observ, UK Astron Technol Ctr, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
[2] Royal Observ, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
[3] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[4] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[5] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[6] Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
[7] Univ Arizona, Steward Observ, Tucson, AZ 85718 USA
[8] Leiden Univ, Sterrewacht Leiden, NL-2300 RA Leiden, Netherlands
[9] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
来源
关键词
Solar system: origin and evolution; Accretion and accretion disks; Mass loss and stellar winds; Protostars; Infrared excess; debris disks; protoplanetary disk; Atomic; molecular; chemical; and grain processes; HIGH-RESOLUTION SPECTROSCOPY; MOLECULAR-HYDROGEN EMISSION; NE-II EMISSION; STARS; DISCS; PHOTOEVAPORATION; TEMPERATURE; ACCRETION; NEARBY; MODELS;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This article summarizes a Splinter Session at the Cool Stars XV conference in St. Andrews with 3 review and 4 contributed talks. The speakers have discussed various approaches to understand the structure and evolution of the gas component in protoplanetary disks. These ranged from observational spectroscopy in the UV, infrared and millimeter, through to chemical and hydrodynamical models. The focus was on disks around low-mass stars, ranging from classical T Tauri stars to transitional disks and debris disks. Emphasis was put on water and organic molecules, the relation to planet formation, and the formation of holes and gaps in the inner regions.
引用
收藏
页码:225 / +
页数:2
相关论文
共 50 条
  • [21] The Evolution of the Inner Regions of Protoplanetary Disks
    Manzo-Martinez, Ezequiel
    Calvet, Nuria
    Hernandez, Jesus
    Lizano, Susana
    Hernandez, Ramiro Franco
    Miller, Christopher J.
    Mauco, Karina
    Briceno, Cesar
    D'Alessio, Paola
    ASTROPHYSICAL JOURNAL, 2020, 893 (01):
  • [22] Dust evolution in protoplanetary accretion disks
    Henning, T
    Schmitt, W
    Mucha, R
    ACCRETION PHENOMENA AND RELATED OUTFLOWS: IAU COLLOQUIUM 163, 1997, 121 : 721 - 722
  • [23] EARLY STAGES IN THE EVOLUTION OF PROTOPLANETARY DISKS
    Hernandez, J.
    Calvet, N.
    Hartmann, L.
    Briceno, C.
    Vivas, A. K.
    Muzerolle, J.
    Gutermuth, R.
    XII IAU REGIONAL LATIN AMERICAN MEETING, 2009, 35 : 68 - +
  • [24] Dust evolution in protoplanetary accretion disks
    Schmitt, W
    Henning, T
    Mucha, R
    ASTRONOMY & ASTROPHYSICS, 1997, 325 (02) : 569 - 584
  • [25] PROTOPLANETARY GAS DISKS IN THE FAR INFRARED
    Goicoechea, Javier R.
    Swinyard, Bruce
    SPICA JOINT EUROPEAN/JAPANESE WORKSHOP, 2009,
  • [26] Observational Diagnostics of Gas in Protoplanetary Disks
    Andrés Carmona
    Earth, Moon, and Planets, 2010, 106 : 71 - 95
  • [27] Cold CO gas in protoplanetary disks
    Aikawa, Yuri
    ASTROPHYSICAL JOURNAL, 2007, 656 (02): : L93 - L96
  • [28] Thermal evolution of protoplanetary disks: from β-cooling to decoupled gas and dust temperatures
    Vorobyov, Eduard I.
    Matsukoba, Ryoki
    Omukai, Kazuyuki
    Guedel, Manuel
    ASTRONOMY & ASTROPHYSICS, 2020, 638
  • [29] Consistent dust and gas models for protoplanetary disks IV. A panchromatic view of protoplanetary disks
    Dionatos, O.
    Woitke, P.
    Guedel, M.
    Degroote, P.
    Liebhart, A.
    Anthonioz, F.
    Antonellini, S.
    Baldovin-Saavedra, C.
    Carmona, A.
    Dominik, C.
    Greaves, J.
    Ilee, J. D.
    Kamp, I
    Menard, F.
    Min, M.
    Pinte, C.
    Rab, C.
    Rigon, L.
    Thi, W. F.
    Waters, L. B. F. M.
    ASTRONOMY & ASTROPHYSICS, 2019, 625
  • [30] ON THE EVOLUTION OF THE CO SNOW LINE IN PROTOPLANETARY DISKS
    Martin, Rebecca G.
    Livio, Mario
    ASTROPHYSICAL JOURNAL LETTERS, 2014, 783 (02)