Chasing disk dispersal indicators: The origin of the [OI] low-velocity components from young stars

Elisabetta Rigliaco, Ilaria Pascucci, Uma Gorti, Suzan Edwards, David Holenbach

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Understanding how a disk surrounding a young star evolves and disperses is crucial in order to understand the subsequent planet formation. In this proceeding, we summarize the results reported by Rigliaco et al. (2013) on the origin of the [OI] low-velocity component as a possible disk dispersal indicator.

Original languageEnglish (US)
Title of host publicationExploring the Formation and Evolution of Planetary Systems
PublisherCambridge University Press
Pages226-227
Number of pages2
EditionS299
ISBN (Print)9781107045200
DOIs
StatePublished - Jun 2013

Publication series

NameProceedings of the International Astronomical Union
NumberS299
Volume8
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • Accretion
  • Accretion disks - stars: formation - planetary systems:protoplanetary disks - stars: pre-main-sequence - ultraviolet:stars

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

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  • Cite this

    Rigliaco, E., Pascucci, I., Gorti, U., Edwards, S., & Holenbach, D. (2013). Chasing disk dispersal indicators: The origin of the [OI] low-velocity components from young stars. In Exploring the Formation and Evolution of Planetary Systems (S299 ed., pp. 226-227). (Proceedings of the International Astronomical Union; Vol. 8, No. S299). Cambridge University Press. https://doi.org/10.1017/S1743921313008430