TY - GEN
T1 - Chasing disk dispersal indicators
T2 - The origin of the [OI] low-velocity components from young stars
AU - Rigliaco, Elisabetta
AU - Pascucci, Ilaria
AU - Gorti, Uma
AU - Edwards, Suzan
AU - Holenbach, David
PY - 2013/6
Y1 - 2013/6
N2 - 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.
AB - 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.
KW - Accretion
KW - Accretion disks - stars: formation - planetary systems:protoplanetary disks - stars: pre-main-sequence - ultraviolet:stars
UR - http://www.scopus.com/inward/record.url?scp=84891857019&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84891857019&partnerID=8YFLogxK
U2 - 10.1017/S1743921313008430
DO - 10.1017/S1743921313008430
M3 - Conference contribution
AN - SCOPUS:84891857019
SN - 9781107045200
T3 - Proceedings of the International Astronomical Union
SP - 226
EP - 227
BT - Exploring the Formation and Evolution of Planetary Systems
PB - Cambridge University Press
ER -