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A revised effective-temperature calibration for the DDO photometric system A revised effective-temperature calibration for the David DunlapObservatory (DDO) photometric system is presented. Recently publishedphotometric and spectroscopic observations of field and open-cluster Gand K stars allow a better definition of the solar-abundance fiducialrelation in the DDO C0(45-48) vs. C0(42-45)diagram. The ability of the DDO system to predict MK spectral types of Gand K giants is demonstrated. The new DDO effective temperaturecalibration reproduces satisfactorily the infrared temperature scale ofBell and Gustafsson (1989). It is shown that Osborn's (1979) calibrationunderestimates the effective temperatures of K giants by approximately170 K and those of late-type dwarfs by approximately 150 K.
 
  |  Untersuchungen an Farbenindizes II. Mit 1 Textabbildung Not Available
 
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Osservazione e dati astrometrici
| Costellazione: | Carena |  
    | Ascensione retta: | 10h23m05.19s |  
    | Declinazione: | -61°15'56.4" |  
    | Magnitudine apparente: | 7.489 |  
    
        | Distanza: | 613.497 parsec |  
        
    
    | Moto proprio RA: | -9 |  
    | Moto proprio Dec: | 6.8 |  
    | B-T magnitude: | 9.106 |  
    | V-T magnitude: | 7.623 |  
    
 
 
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