The Future of High Angular Resolution Star and Planet Formation Science in the Optical/Infrared
Astrophysics
2007-05-23 v1
Abstract
This presentation summarizes how some of the most pressing questions in the field of star and planet formation can be addressed by high angular resolution optical/infrared capabilities, and how many of these capabilities will in fact be available with realization of the space and ground facilities currently being planned for the 2005-2020 time frame.
Cite
@article{arxiv.astro-ph/0312188,
title = {The Future of High Angular Resolution Star and Planet Formation Science in the Optical/Infrared},
author = {Lynne A. Hillenbrand},
journal= {arXiv preprint arXiv:astro-ph/0312188},
year = {2007}
}
Comments
9 pages, 0 figures; to appear in "Star Formation at High Angular Resolution" (IAU 221) edited by M.G. Burton, R. Jayawardhana, and T.L. Bourke (2004)