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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.
 
  |  Radial-velocity measurements. V - Ground support of the HIPPARCOS satellite observation program The paper presents data on 1070 radial velocity measurements of starsdistributed in 39 fields measuring 4 deg x 4 deg. The PPO series ofFehrenbach et al. (1987) and Duflot et al. (1990) is continued using theFehrenbach objective prism method.
 
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Zincirli Prenses |  
    | Sað Açýklýk: | 00h48m02.01s |  
    | Yükselim: | +52°16'31.0" |  
    | Görünürdeki Parlaklýk: | 8.481 |  
    
        | Uzaklýk: | 259.74 parsek |  
        
    
    | özdevim Sað Açýklýk: | -9.6 |  
    | özdevim Yükselim: | 0 |  
    | B-T magnitude: | 8.86 |  
    | V-T magnitude: | 8.513 |  
    
 
 
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