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Kinematics of Hipparcos Visual Binaries. I. Stars with Orbital Solutions
A sample consisting of 570 binary systems is compiled from severalsources of visual binary stars with well-known orbital elements.High-precision trigonometric parallaxes (mean relative error about 5%)and proper motions (mean relative error about 3%) are extracted from theHipparcos Catalogue or from the reprocessed Hipparcos data. However, 13%of the sample stars lack radial velocity measurements. Computed galacticvelocity components and other kinematic parameters are used to dividethe sample stars into kinematic age groups. The majority (89%) of thesample stars, with known radial velocities, are the thin disk stars,9.5% binaries have thick disk kinematics and only 1.4% are halo stars.85% of thin disk binaries are young or medium age stars and almost 15%are old thin disk stars. There is an urgent need to increase the numberof the identified halo binary stars with known orbits and substantiallyimprove the situation with their radial velocity data.
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Agcik |
| Sað Açýklýk: | 03h32m00.71s |
| Yükselim: | -65°38'43.5" |
| Görünürdeki Parlaklýk: | 8.241 |
| Uzaklýk: | 343.643 parsek |
| özdevim Sað Açýklýk: | 14 |
| özdevim Yükselim: | 0.5 |
| B-T magnitude: | 9.879 |
| V-T magnitude: | 8.377 |
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