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The companion object to HD114762We obtained 28 independent radial velocity measurements on the star HD114762, and are now able to derive orbit solution. We confirm the existence of a companion object in an orbit with a semimajor axis about 0.4 au. The new orbit solution is discussed. The result show that the companion is not a planet, but instead is a brown dwarf or a low mass star in a system viewed nearly pole-on.
Document ID
19920003647
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Cochran, William D. (McDonald Observatory Austin, TX, United States)
Date Acquired
September 6, 2013
Publication Date
October 1, 1991
Publication Information
Publication: NASA, Washington, Reports of Planetary Astronomy, 1991
Subject Category
Astronomy
Accession Number
92N12865
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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