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High Spatial Resolution Imaging of Pre-Main-Sequence Binary Stars: Resolving the Relationship between Disks and Close Companions
- Source :
- The Astrophysical Journal; November 1997, Vol. 490 Issue: 1 p353-367, 15p
- Publication Year :
- 1997
-
Abstract
- In order to study the passive and active effects of young close companion stars and to constrain possible multiple star formation mechanisms, we have carried out a high-resolution imaging program of six multiple T Tauri star systems using the HubbleSpaceTelescope from 0.3 to 0.9 ?m and ground-based speckle imaging from 1 to 2 ?m. Each system (GG Tau, UZ Tau, DF Tau, RW Aur, V773 Tau, and V410 Tau) has at least one binary pair with separation between 007 and 04 (10-50 AU). In addition to the previously known companions, a third component is discovered in the V410 Tau system.
Details
- Language :
- English
- ISSN :
- 0004637X and 15384357
- Volume :
- 490
- Issue :
- 1
- Database :
- Supplemental Index
- Journal :
- The Astrophysical Journal
- Publication Type :
- Periodical
- Accession number :
- ejs56556064
- Full Text :
- https://doi.org/10.1086/304856