High-contrast Polarimetry Observation of the T Tau Circumstellar Environment
Hayashi, Saeko S.
Brandt, Timothy D.
Carson, Joseph C.
Grady, Carol A.
Hodapp, Klaus W.
Knapp, Gillian R.
McElwain, Michael W.
Takahashi, Yasuhiro H.
Turner, Edwin L.
AffiliationUniv Arizona, Steward Observ
binaries: general (T Tau)
stars: pre-main sequence
stars: variables: T Tauri, Herbig Ae/Be
MetadataShow full item record
PublisherIOP PUBLISHING LTD
CitationYi Yang et al 2018 ApJ 861 133
Rights© 2018. The American Astronomical Society. All rights reserved.
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AbstractWe conducted high-contrast polarimetry observations of T Tau in the H-band, using the High Contrast Instrument for the Subaru Next Generation Adaptive Optics instrument mounted on the Subaru Telescope, revealing structures as near as 0 1 from the stars T Tau N and T Tau S. The whole T Tau system is found to be surrounded by nebulalike envelopes, and several outflow-related structures are detected in these envelopes. We analyzed the detailed polarization patterns of the circumstellar structures near each component of this triple young star system and determined constraints on the circumstellar disks and outflow structures. We suggest that the nearly face-on circumstellar disk of T Tau N is no larger than 0.''8, or 117 au, in the northwest, based on the existence of a hole in this direction, and no larger than 0.''27, or 40 au, in the south. A new structure, "N5," extends to about 0.''42, or 59 au, southwest of the star, and is believed to be part of the disk. We suggest that T Tau S is surrounded by a highly inclined circumbinary disk with a radius of about 0.''3, or 44 au, with a position angle of about 30 degrees, that is misaligned with the orbit of the T Tau S binary. After analyzing the positions and polarization vector patterns of the outflow-related structures, we suggest that T Tau S should trigger the well-known E-W outflow, and is also likely to be responsible for a southwest precessing outflow "coil" and a possible south outflow.
VersionFinal published version
SponsorsU.S. National Science Foundation ; [15H02063]