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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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Osservazione e dati astrometrici
| Costellazione: | Gemelli |  
    | Ascensione retta: | 07h17m57.36s |  
    | Declinazione: | +28°29'18.7" |  
    | Magnitudine apparente: | 8.394 |  
    
        | Distanza: | 130.719 parsec |  
        
    
    | Moto proprio RA: | -49.2 |  
    | Moto proprio Dec: | -51 |  
    | B-T magnitude: | 8.981 |  
    | V-T magnitude: | 8.443 |  
    
 
 
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