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- W60780129 abstract "We have recently reported the discovery of a cool (650–800 K) low-luminosity companion to the pre-main-sequence star, T Tauri (Dyck et al. 1982). We proposed that the optical star and its infrared companion form a physical pair with a N-S separation of 100 a.u. However, there remained in our 2–5 μm speckle interferometry an ambiguity of 180° in the position angle of the secondary. In addition, Cohen et al. (1982) noted an 800 milliarcsec (mas) offset between the visual and 6 cm radio positions at T Tau. Both of these positional discrepancies have now been clarified by accurate visual and radio astrometry of T Tau, and by further near-IR speckle interferometry." @default.
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- W60780129 date "1983-01-01" @default.
- W60780129 modified "2023-09-24" @default.
- W60780129 title "New Results on the Binary Companion of T Tauri" @default.
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- W60780129 doi "https://doi.org/10.1007/978-94-009-7157-8_72" @default.
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