The Future of High Angular Resolution Star and Planet Formation Science in the Optical/Infrared
| dc.creator | Hillenbrand, Lynne A. | |
| dc.date | 2003-12-06 | |
| dc.date.accessioned | 2026-07-07T02:11:28Z | |
| dc.date.available | 2026-07-07T02:11:28Z | |
| dc.description | 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. | |
| dc.description | 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) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0312188 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0312188 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7101 | |
| dc.subject | Astrophysics | |
| dc.title | The Future of High Angular Resolution Star and Planet Formation Science in the Optical/Infrared | |
| dc.type | text |