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Spectroscopic binaries in the Orion OB1 association
A radial velocity study of the brighter members of the Ori OB2association is reported. The radial velocity variables, new preliminaryorbital elements for six spectroscopic binaries, and the projected axialrotation in stars for which the orbital elements are lacking arereported. The correlation between the proportion of binaries and theaverage axial rotation for the subgroups of the association isdiscussed. It is found that the Orion main-sequence members rotate atalmost the same rate as field stars of the same types. The averageradial velocity for the whole association is 23 km/s. The percentage ofspectroscopic binaries with periods shorter than 100 days plus themagnetic Ap-Bp among the main-sequence members of the association is 32percent.
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| Takýmyýldýz: | Avci |
| Sað Açýklýk: | 05h27m13.82s |
| Yükselim: | +04°10'24.7" |
| Görünürdeki Parlaklýk: | 9.698 |
| özdevim Sað Açýklýk: | -0.3 |
| özdevim Yükselim: | -10.2 |
| B-T magnitude: | 9.942 |
| V-T magnitude: | 9.719 |
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