@inproceedings{8c72e7ec1a33422682ee9efceaf6de0e,
title = "Evolution and Dispersal of Protoplanetary Disks",
abstract = "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.",
keywords = "Stars: Formation, Planetary systems: Protoplanetary disks, Accretion disks, T-TAURI STARS, INTERSTELLAR SILICATE MINERALOGY, SPITZER-SPACE-TELESCOPE, ACCRETION, DUST, PLANET, PHOTOEVAPORATION, GROWTH, GRAINS, MODELS",
author = "A. Sicilia-Aguilar and Th. Henning and A. Juhasz and J. Bouwman and L. Hartmann and D. Watson",
year = "2009",
language = "English",
isbn = "978-0-7354-0627-8",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics",
pages = "23--28",
editor = "E Stempels",
booktitle = "COOL STARS, STELLAR SYSTEMS AND THE SUN",
address = "United States",
note = "15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun ; Conference date: 21-07-2008 Through 25-07-2008",
}