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A homogeneous catalog of new UBV and H-beta photometry of B- and A-type stars in and around the Scorpius-Centaurus OB association B- and A-type stars in and near the Sco-Cen OB association areinvestigated with UBV and H-beta photometry to acquire data relevant tothe luminosity function of Sco-Cen. The measurements generally consistof two 10-s integrations of U, B, V, (W, N) filters, and theobservations are corrected iteratively for atmospheric extinction andinstrumental response. The data presented give the mean V magnitude,mean B-V, mean U-B, and the estimated uncertainties for these values.The catalog provides a homogeneous catalog of data for a large fieldwith stellar objects delineating membership to the association Sco-Cenand that affect the luminosity function of the aggregate.
 
  |  The chemical evolution of the solar neighborhood. I - A bias-free reduction technique and data sample The possible ways of measuring the age-metallicity relation for thegalactic disk in the neighborhood of the sun are discussed. It is shownthat the use of a field star sample chosen on the basis of effectivetemperature introduces a bias which results in a monotonic increase inthe metal abundance of the disk with time. However, if theage-metallicity relation for the disk can be shown to satisfy certaincriteria, the bias introduced in such a sample can be neglected: thegalactic disk apparently satisfies the criteria. It is concluded that asample analyzed through the use of uvby and H(beta) photometry inconjunction with a self-consistent set of theoretical isochronesprovides the least biased, most accurate estimate of the age-metallicityrelation for the disk.
 
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 Miembro de los siguientes grupos:
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Datos observacionales y astrométricos
| Constelación: | Mosca |  
    | Ascensión Recta: | 13h11m45.29s |  
    | Declinación: | -68°55'00.9" |  
    | Magnitud Aparente: | 7.977 |  
    
        | Distancia: | 395.257 parsecs |  
        
    
    | Movimiento Propio en Ascensión Recta: | 6.7 |  
    | Movimiento Propio en Declinación: | 1.8 |  
    | B-T magnitude: | 8.407 |  
    | V-T magnitude: | 8.013 |  
    
 
 
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