Issue |
A&A
Volume 593, September 2016
|
|
---|---|---|
Article Number | A50 | |
Number of page(s) | 8 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201527818 | |
Published online | 15 September 2016 |
New circumstellar structure in the T Tauri system
A near-infrared high-contrast imaging study
1 European Southern Observatory
(ESO), Karl-Schwarzschild-Str.
2, 85748 Garching, Germany
e-mail: mkasper@eso.org
2 Max-Planck-Institute for Astronomy
(MPIA), Königstuhl
17, 69117
Heidelberg,
Germany
3 International Max Planck Research School for Astronomy and
Cosmic Physics at the University of Heidelberg, Germany
4 Universität Innsbruck, Institut für
Astro- und Teilchenphysik, Technikerstr. 25/8, 6020
Innsbruck,
Austria
5 University of Vienna, Department of
Astrophysics, Türkenschanzstr. 17
(Sternwarte), 1180
Vienna,
Austria
Received:
24
November
2015
Accepted:
18
May
2016
Aims. The immediate vicinity of T Tauri was observed with the new high-contrast imaging instrument SPHERE at the VLT to resolve remaining mysteries of the system, such as the putative small edge-on disk around T Tauri Sa and the assignment of the complex outflow patterns to the individual stars.
Methods. We used SPHERE IRDIS narrow-band classical imaging in Paβ, Brγ, and the ν = 1−0 S(1) line of H2, as well as in the nearby continua to obtain high spatial resolution and high-contrast images over the near-infrared spectral range. Line maps were created by subtracting the nearby continuum. We also reanalyzed coronagraphic data taken with SPHERE’s integral field spectrograph in J- and H-band with the goal of obtaining a precise extinction estimate to T Tauri Sb, and of verifying the recently reported claim of another stellar or substellar object in the system.
Results. A previously unknown coiling structure is observed southwest of the stars in reflected light, which points to the vicinity of T Tauri N. We map the circumbinary emission from T Tauri S in J- and H-band scattered light for the first time, showing a morphology that differs significantly from that observed in K-band. Molecular Hydrogen emission is found southwest of the stars, near the coiling structure. We also detect the H2 emitting region T Tauri NW. The motion of T Tauri NW with respect to T Tauri N and S between previous images and our 2014 data provides strong evidence that the southeast–northwest outflow triggering T Tauri NW is likely to be associated with T Tauri S. We also present accurate relative photometry of the stars, which confirms that T Tauri Sa is brightening again. Our analysis rules out the presence of the recently proposed companion to T Tauri N with high confidence.
Key words: techniques: high angular resolution / stars: formation / stars: individual: T Tauri / stars: winds, outflows
© ESO, 2016
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