Near-Infrared Coronagraphic Observations of a Classical TTauri Star, DO Taurus

Details Near-Infrared Coronagraphic Observations of a Classical TTauri Star, DO Taurus Near-Infrared Coronagraphic Observations of a Classical TTauri Star, DO Taurus

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008pasj...60..223i&link_type=abstract

Publications of the Astronomical Society of Japan, Vol.60, No.2, pp.223--226

Astronomy and Astrophysics

Astronomy

1

Stars: Individual (Do Taurus), Stars: Pre-Main Sequence, Techniques: High Angular Resolution

Scientific paper

A high angular resolution near-infrared image of a classical TTauri star, DO Tau, was obtained with Coronagraphic Imager with Adaptive Optics (CIAO) mounted on the Subaru Telescope. Circumstellar emission was detected at ˜1".7 from the central star in the direction of the redshifted jet. No emission was found toward the opposite direction. We also found one faint point source 3".46 away from the central star. The following observation will reveal whether it is an associated planetary mass object or a background object.

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