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Photometry of F-K type bright giants and supergiants. I - Intermediate band and H-Beta observations
Over 1500 observations of 560 bright giants and supergiants of types F-Kare presented and compared to the observations by Gray and Olsen (1991).The present results include intermediate-band which is slightlydifferent from the Stromgren data by Gray and Olsen due to a differentwidth for the v filter. A systematic difference in m(1) - M(1) withdecreasing temperature is noted in the two H-Beta data sets, and thecorrelations are defined.

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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Dades d'Observació i Astrometria

Constel·lació:Lupus
Ascensió Recta:15h17m53.12s
Declinació:-52°17'11.4"
Magnitud Aparent:8.164
Distancia:490.196 parsecs
Moviment propi RA:-15
Moviment propi Dec:-6.2
B-T magnitude:9.62
V-T magnitude:8.285

Catàlegs i designacions:
Noms Propis   (Edit)
HD 1989HD 135551
TYCHO-2 2000TYC 8306-118-1
USNO-A2.0USNO-A2 0375-24010437
HIPHIP 74859

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