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Three colour observations of southern red variable giant stars
UBV observations have been made of southern red variables of varioustypes over a period of two years. Accurate light curves of about 35variables have been obtained; in many cases the observations coveredmore than one cycle. It appears that the M-type SRb and Lb variablesdefine a curved strip in the (B-V)-(U-B) plane. The mean (U-B) of thevariable stars is about 0.5 mag bluer than the (U-B) of the nonvariableK-type giants. The red variables may be divided into different groups:the carbon stars and the M-type variables, of which the M-type stars areagain to be divided into three groups on the basis of their colorvariations and consequently their loops in the two-color plane.
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Tavsan |
| Sað Açýklýk: | 05h12m16.44s |
| Yükselim: | -11°48'10.6" |
| Görünürdeki Parlaklýk: | 8.161 |
| Uzaklýk: | 99.01 parsek |
| özdevim Sað Açýklýk: | 76.4 |
| özdevim Yükselim: | 15.2 |
| B-T magnitude: | 8.74 |
| V-T magnitude: | 8.209 |
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