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- W2140770443 abstract "For at all 24 stars in the field of the heavity reddened open cluster NGC 1502 we obtained UBV and uvby photometry. 19 of these stars we classified definitely as members. From the photometric results we derived 1·1 × 107 years as the cluster age, 960 pc as its distance, and = 0·78 mag as mean reddening of the cluster. From the reddening of the foreground stars we evaluated that the intracluster reddening has to be smaller than 0·2 mag. The value of the colour excess ratio E(b—y)/E(B—V) = 0·770 leads us to the conclusion that in the spectra of the cluster stars a very broadband structure (VBS) with a central depth of about 0·04 mag is present.Fur insgesamt 24 Sterne im Gebiet des stark verfarbten offenen Haufens NGC 1502 erhielten wir UBV und uvby Photometrie, Neunzehn dieser Sterne konnten wir definitiv als Haufenmitglieder klassifizieren. Aus der Photometrie leiteten wir ein Haufenalter von 1·1 × 107 Jahren, eine Entfernung von 960 pc und eine Verfarbung = 0·78 mag ab. Aus der Verfarbung der Vordergrundsterne kann man abschatzen, das der Farbexzess innerhalb des Haufens kleiner als 0·2 mag sein mus. Aus der Grose des Farbexzessverhaltnisses E(b—y)/E(B—V) = 0·770 schliesen wir auf eine Starke der Breitbandstruktur (VBS) von 0·04 mag." @default.
- W2140770443 created "2016-06-24" @default.
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- W2140770443 date "1987-01-01" @default.
- W2140770443 modified "2023-09-25" @default.
- W2140770443 title "CombinedUBV anduvby photometry of open clusters. I. NGC 1502" @default.
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- W2140770443 doi "https://doi.org/10.1002/asna.2113080206" @default.
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