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HD 3566


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A survey of proper-motion stars. VI - Orbits for 40 spectroscopic binaries
Orbital solutions are reported for 40 binaries in the Carney and Latham(1987) survey of proper-motion stars. The earlier orbital solutions forHD 85091, BD + 13 3683 deg, and HD 195987 are confirmed, and that for BD-3 2525 deg is revised. The number of orbital solutions for metal-poorbinaries has been increased from five to 19, six of which have doublelines. For periods longer than 20 days, the distribution of orbitaleccentricity for the metal-poor binaries is similar to that for themetal-rich binaries. For the metal-poor binaries, it is found that allthe short-period orbits are circular, with a transition to eccentricorbits at a period somewhere between 13 and 18 days. Presumably, theclose binaries with short periods were formed with eccentric orbitswhich were subsequently circularized by tidal mechanisms.

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Datos observacionales y astrométricos

Constelación:Ballena
Ascensión Recta:00h38m40.33s
Declinación:+00°39'13.9"
Magnitud Aparente:9.969
Movimiento Propio en Ascensión Recta:49.6
Movimiento Propio en Declinación:-12.1
B-T magnitude:10.718
V-T magnitude:10.031

Catálogos y designaciones:
Nombres Propios   (Edit)
HD 1989HD 3566
TYCHO-2 2000TYC 10-323-1
USNO-A2.0USNO-A2 0900-00151188

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