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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.
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| Сазвежђа: | Шестар |
| Ректацензија: | 14h26m48.81s |
| Deклинација: | -67°24'46.8" |
| Apparent магнитуда: | 8.211 |
| Даљина: | 403.226 parsecs |
| Proper motion RA: | -2.1 |
| Proper motion Dec: | -2.1 |
| B-T magnitude: | 10.377 |
| V-T magnitude: | 8.39 |
Каталог и designations:
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