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arXiv · 1205.5760

A Proper Motion Study of the Haro 6-10 Outflow: Evidence for a Subarcsecond Binary

Bruce A. Wilking·Kevin B. Marvel·Mark J. Claussen·Bradley M. Gerling·Alwyn Wootten·Erika Gibb
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Abstract

We present single-dish and VLBI observations of an outburst of water maser emission from the young binary system Haro 6-10. Haro 6-10 lies in the Taurus molecular cloud and contains a visible T Tauri star with an infrared companion 1.3" north. Using the Very Long Baseline Array, we obtained five observations spanning 3 months and derived absolute positions for 20 distinct maser spots. Three of the masers can be traced over 3 or more epochs, enabling us to extract absolute proper motions and tangential velocities. We deduce that the masers represent one side of a bipolar outflow that lies nearly in the plane of the sky with an opening angle of ~45°. They are located within 50 mas of the southern component of the binary, the visible T Tauri star Haro 6-10S. The mean position angle on the sky of the maser proper motions (~220°) suggests they are related to the previously observed giant Herbig-Haro (HH) flow which includes HH410, HH411, HH412, and HH184A-E. A previously observed HH jet and extended radio continuum emission (mean position angle of ~190°) must also originate in the vicinity of Haro6-10S and represent a second, distinct outflow in this region. We propose that a yet unobserved companion within 150 mas of Haro6-10S is responsible for the giant HH/maser outflow while the visible star is associated with the HH jet. Despite the presence of H_2 emission in the spectrum of the northern component of the binary, Haro6-10N, none of outflows/jets can be tied directly to this young stellar object.

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Bruce A. Wilking, Kevin B. Marvel, Mark J. Claussen, Bradley M. Gerling, Alwyn Wootten, Erika Gibb. 2012-05-25. A Proper Motion Study of the Haro 6-10 Outflow: Evidence for a Subarcsecond Binary. https://doi.org/10.1088/0004-637x%2F753%2F2%2F143

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