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Photometry of possible members of the Hyades cluster. V
Photoelectric BVRI observations have been obtained for 36 starssuspected of being members of the Hyades cluster, mostly on the basis ofthe proper-motion survey by Artyukhina and Kholopov. Most of the starsare in the outer regions of the cluster and, on the basis of thephotometry, only six of the 36 stars appear to be possible or probablemembers. This illustrates the difficulty of identifying outlying clustermembers on the basis of proper-motion measures alone.
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Boga |
| Sað Açýklýk: | 05h16m37.37s |
| Yükselim: | +21°13'56.8" |
| Görünürdeki Parlaklýk: | 10.369 |
| özdevim Sað Açýklýk: | 52.3 |
| özdevim Yükselim: | -30.7 |
| B-T magnitude: | 11.218 |
| V-T magnitude: | 10.44 |
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