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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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| Сазвежђа: | Пегаз |
| Ректацензија: | 22h07m38.99s |
| Deклинација: | +25°00'58.2" |
| Apparent магнитуда: | 8.302 |
| Даљина: | 171.527 parsecs |
| Proper motion RA: | 16.9 |
| Proper motion Dec: | -12.4 |
| B-T magnitude: | 8.679 |
| V-T magnitude: | 8.334 |
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