The Disk and Jet Structure of Holoea

Details The Disk and Jet Structure of Holoea The Disk and Jet Structure of Holoea

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6459m&link_type=abstract

HST Proposal ID #6459

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Hst Proposal Id #6459 Cool Stars

Scientific paper

We have discovered an object in the field of the Galactic opencluster M36 which exhibits a nebulous tail-like structure, abipolar molecular outflow, a high-velocity ionized wind, and abright central star with spectral type ~ K0 III (Magnier et al.,1995). This source, which we have nick-named ``Holoea'', mostlikely represents a very early stage in the evolution fromembedded to naked T Tauri star. It also presents an unusualopportunity to study a stellar jet from two angles at oncebecause of a fortuitous reflection off of the nebulous tail.For these reasons, we are vigorously pursuing a program tostudy this system in detail. Here, we propose to take high-resolution optical images to study the jet andaccretion disk structures, both directly and through thereflection. We also hope to find HH objects or other knots inthe outflow, which will allow us eventually to measure thedistance to the object via proper motion.

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