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- W3105090468 abstract "We present a UBV CCD photometric study of four open clusters, NGC 7245, King 9, IC 166 and King 13, located between l= 90° and 135°. All are embedded in a rich Galactic field. NGC 7245 and King 9 are close together in the sky and have similar reddenings. The distances and ages are: NGC 7245, 3.8 ± 0.35 kpc and 400 Myr; King 9 (the most distant cluster in this quadrant), 7.9 ± 1.1 kpc and 3.0 Gyr. King 13 is 3.1 ± 0.3 kpc distant and 300 Myr old. King 9 and IC 166 (4.8 ± 0.5 kpc distant and 1 Gyr old) may be metal-poor clusters (Z= 0.008), as estimated from isochrone fitting. The average value of the distance of young clusters from the Galactic plane in the above longitude range and beyond 2 kpc (−47 ± 16 pc, for 64 clusters) indicates that the young disc bends towards the southern latitudes." @default.
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- W3105090468 date "2007-05-11" @default.
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- W3105090468 title "Photometric study of distant open clusters in the second quadrant: NGC 7245, King 9, King 13 and IC 166" @default.
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- W3105090468 doi "https://doi.org/10.1111/j.1365-2966.2007.11648.x" @default.
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