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The reddening, metal abundance, and luminosity of high-luminosity G-type stars
The abundance parameters of the sample of 100 G-type bright giants andsupergiants whose photometry is presently discussed indicate Fe/H valuesof between about + 0.6 dex and the solar value, using a preliminarycalibration of the photometric indices. The few long period Cepheidsthat are not heavily blanketed F-type stars give reddening values thatare in agreement with current results from other methods of analysis.Supergiants show no clear gradients in the galactic distribution ofabundances, and those nearest the sun range from an Fe/H of about + 0.3dex, for members of the Pleiades Group, to near solar abundance. A smallsample of Large Magellanic Cloud supergiants shows nearly the same rangein metal abundance as the galactic stars, and gives a modulus for thisCloud of 18.3 + or - 0.20 mag.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Crux |
| Ascensió Recta: | 12h04m32.72s |
| Declinació: | -63°34'38.0" |
| Magnitud Aparent: | 8.035 |
| Distancia: | 317.46 parsecs |
| Moviment propi RA: | -8.1 |
| Moviment propi Dec: | -3.3 |
| B-T magnitude: | 9.655 |
| V-T magnitude: | 8.169 |
Catàlegs i designacions:
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INHABITED SKY
