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2008BaltA..17..103B - Baltic Astronomy, 17, 103-111 (2008/April-0)
High velocity spectroscopic binary orbits from photoelectric radial velocities: A triple system BD+39 1828.
BARTKEVICIUS A., BOYLE R.P. and SPERAUSKAS J.
Abstract (from CDS):
Spectroscopic orbit of the component A of the orbital visual binary BD+39 1828 is calculated using 27 CORAVEL-type radial velocity measurements. A circular orbit with the period P = 5.28 days is obtained. The primary component of the spectroscopic binary is a K4V star and the secondary is an M dwarf. The component B of the visual pair is a K5V star. The binary has the solar chemical composition and kinematically belongs to the old thin disk population of the Galaxy.
Abstract Copyright: ∼
Journal keyword(s): stars: binaries: spectroscopic, visual, individual (BD+39 1828)
Simbad objects: 1
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