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Uvby-beta observations of 528 type B stars with V between the 8th and 9th magnitude The paper presents uvby-beta measurements of 528 type B stars selectedfrom the SAO Catalog on the basis of two criteria: the spectral types inthe range B3-B5 and mV between the 8th and the 9th magnitude. Reddeningindependent (c1) values are estimated from the spectral classificationand compared to the observed values. No systematic trend with observed(b-y), H-beta, or spectral type appears to be present, but the range of(c1) residuals is surprisingly large. A rather large part of the starshas small beta values, smaller than for the BIa supergiants. Only twoare classified as O stars and most of them have the suffix e, ne, ornne. Most beta values for the O type stars are slightly above the upperlimit of 2.585 m.
 
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Yilanci |  
    | Sað Açýklýk: | 17h33m36.55s |  
    | Yükselim: | -07°29'20.5" |  
    | Görünürdeki Parlaklýk: | 9.943 |  
    
    
    | özdevim Sað Açýklýk: | -3.1 |  
    | özdevim Yükselim: | -4.1 |  
    | B-T magnitude: | 10.632 |  
    | V-T magnitude: | 10 |  
    
 
 
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