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A Candidate Protoplanet in the Taurus Star Forming RegionA long narrow filament seems to connect the protobinary to the faint companion TMR-1C, suggesting a physical association. If the sources are physically related then we hypothesize that TMR-1C has been ejected by the protobinary.
Document ID
20060041575
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/20635
Authors
Terebey, S.
Van Buren, D.
Padgett, D. L.
Hancock, T.
Brundage, M.
Date Acquired
August 23, 2013
Publication Date
October 1, 1998
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
HST/NICMOS faint companion protostar filament protobinary giant planet
circumstella matter planetary systems

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