Abstract
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.
Cite
CITATION STYLE
APA
Koresko, C. D. (2000). A Third Star in the T Tauri System. The Astrophysical Journal, 531(2), L147–L149. https://doi.org/10.1086/312543
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