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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.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Ara |
| Ascensió Recta: | 17h29m16.81s |
| Declinació: | -57°24'42.4" |
| Magnitud Aparent: | 8.007 |
| Distancia: | 344.828 parsecs |
| Moviment propi RA: | -0.7 |
| Moviment propi Dec: | -8 |
| B-T magnitude: | 9.313 |
| V-T magnitude: | 8.115 |
Catàlegs i designacions:
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