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Speckle Observations of Binary Stars with the WIYN Telescope. III. A Partial Survey of A, F, and G Dwarfs
Two hundred thirty nearby main-sequence stars with spectral types in therange of A to G have been observed by way of speckle interferometryusing the WIYN 3.5 m telescope at Kitt Peak, Arizona. The stars had noprevious mention of duplicity in the literature. Of those observed, 14showed clear evidence of a companion, and 63 were classified assuspected nonsingle based on a power spectrum analysis. The remainingstars discussed show no evidence of duplicity to the limit of thedetection system in high-quality observations. The WIYN Observatory is ajoint facility of the University of Wisconsin-Madison, IndianaUniversity, Yale University, and the National Optical AstronomyObservatory.
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Ucgen |
| Sað Açýklýk: | 02h19m19.73s |
| Yükselim: | +33°36'13.7" |
| Görünürdeki Parlaklýk: | 8.193 |
| Uzaklýk: | 298.507 parsek |
| özdevim Sað Açýklýk: | -19 |
| özdevim Yükselim: | -2.7 |
| B-T magnitude: | 8.564 |
| V-T magnitude: | 8.224 |
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