C.D.S. - SIMBAD4 rel 1.7 - 2021.03.05CET10:38:11

2016A&A...593A..50K - Astronomy and Astrophysics, volume 593A, 50-50 (2016/9-1)

New circumstellar structure in the T Tauri system. A near-infrared high-contrast imaging study.


Abstract (from CDS):

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.

Abstract Copyright: © ESO, 2016

Journal keyword(s): techniques: high angular resolution - stars: formation - stars: individual: T Tauri - stars: winds, outflows

CDS comments: Objects R1-R4, C2, C3 not in SIMBAD.

Simbad objects: 4

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Number of rows : 4

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
1 HH 155 HH 04 21 57.1 +19 32 07           ~ 73 1
2 V* T Tau TT* 04 21 59.4323326335 +19 32 06.439974179   11.22 10.12 9.80   K0IV/Ve 1337 1
3 NAME Tau-Aur Complex SFR 04 30 +25.0           ~ 1246 0
4 IRAS 16342-3814 pA* 16 37 39.8700524769 -38 20 17.440442399           ~ 128 0

    Equat.    Gal    SGal    Ecl

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