期刊
ASTROPHYSICAL JOURNAL
卷 531, 期 2, 页码 L147-L149出版社
UNIV CHICAGO PRESS
DOI: 10.1086/312543
关键词
binaries : visual; circumstellar matter; methods : observational; stars : individual (T Tauri); stars : pre-main-sequence
New speckle holographic images of the T Tauri infrared companion (T Tauri IRC; T Tauri S) reveal it to be a double system with a sky-projected separation of 0. 05, corresponding to a linear distance of 7 AU. The presence of this third star may account for the relative paucity of dust surrounding the IRC.
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