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The dwarf spheroidal galaxy in Draco. I - New BV photometry. BV photoelectric photometry for 39 stars and BV photographic photometryfor 514 stars in the field of the Draco dwarf spheroidal galaxy arepresented. The color-magnitude diagram for 512 of these field stars isfound to display a well-defined red horizontal branch as well as a redgiant branch whose observed width is comparable to the accidentalphotometric error. The results also indicate that a more diffusesequence of stars lies about 0.1 mag to the blue of the giant branch andthat an upper horizontal branch of more massive core helium-burningstars may also be present. The foreground reddening toward Draco is thendetermined by narrow-band uvby-beta photometry of galactic B-A-F stars.
 
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Dades d'Observació i Astrometria
| Constel·lació: | Draco |  
    | Ascensió Recta: | 17h20m09.51s |  
    | Declinació: | +51°40'32.0" |  
    | Magnitud Aparent: | 8.125 |  
    
        | Distancia: | 813.008 parsecs |  
        
    
    | Moviment propi RA: | -4.5 |  
    | Moviment propi Dec: | -5.4 |  
    | B-T magnitude: | 9.513 |  
    | V-T magnitude: | 8.24 |  
    
 
 
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