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Some enigmatic binary stars. I
Historical measurements of components of binary star systems at timesexhibit evidence for incompatible interpretations. A short period andstrong eccentricity can equally be a long period with feebleeccentricity. Furthermore, measurements have been made indicating bothdirect and retrograde motions of the components. It has sometimes beenfound that the observations of contradicting evidence have been made ofa second binary system near the system first measured. Note is taken ofthe objects ADS 1959 - A 1818, ADS 2051 - HU 539, ADS 5515 - A 512, ADS5671 - BU 1022, ADS 6001 - A 1963, and ADS 7550 - A 2561, which maypossibly be combinations of two or even three binary clusters observedat different times. Tables are presented of data thus far measured ofeach system.
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Baliklar |
| Sað Açýklýk: | 23h34m14.43s |
| Yükselim: | +02°18'05.5" |
| Görünürdeki Parlaklýk: | 9.46 |
| özdevim Sað Açýklýk: | 81.7 |
| özdevim Yükselim: | -18.2 |
| B-T magnitude: | 10.377 |
| V-T magnitude: | 9.536 |
Kataloglar ve belirtme:
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