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Abstract: From observations collected with the ESPaDOnS and NARVAL spectropolarimeters, we report the detection of Zeeman signatures on the classical T Tauri star (cTTS) BP Tau. Circular polarization ...

Using the speckle camera SHARP at the 3.5m ESO NTT, K\'ohler and collaborators found an object ~3.5 mag fainter in K only 1.3' north-east of the T Tauri star [MR81] Ha 17 in the Corona Australis (CrA) ...

In classical T Tauri stars, the disk does not touch the star directly because it is restricted by the outward pressure of the star's magnetic field. The accretion disks around FU Ori objects ...

In classical T Tauri stars, the disk does not touch the star directly because it is restricted by the outward pressure of the star’s magnetic field. The accretion disks around FU Ori objects, however, ...

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The star is estimated to be about 5 million years old and is assumed to be an intermediate object between a low-mass T Tauri star and a Herbig Ae star. The protoplanetary disk of PDS 453 was first ...