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Chasing disk dispersal indicators: the origin of the [OI] low-velocity components from young stars
Published online by Cambridge University Press: 06 January 2014
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.
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- Contributed Papers
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- Proceedings of the International Astronomical Union , Volume 8 , Symposium S299: Exploring the Formation and Evolution of Planetary Systems , June 2013 , pp. 226 - 227
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- Copyright © International Astronomical Union 2013