Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2199
Title: Photometric study of distant open clusters in the second quadrant: NGC 7245, King 9, King 13 and IC 166
Authors: Subramaniam, A
Bhatt, B. C
Keywords: open clusters and associations: individual: NGC 7245;open clusters and associations: individual: King 9;open clusters and associations: individual: King 13;open clusters and associations: individual: IC 166
Issue Date: May-2007
Publisher: Blackwell Publishing
Citation: MNRAS, Vol. 377, No. 2, pp. 829 - 834
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.
Description: Restricted Access
URI: http://hdl.handle.net/2248/2199
???metadata.dc.relation.uri???: http://www.blackwell-synergy.com/doi/abs/10.1111/j.1365-2966.2007.11648.x
http://arxiv.org/abs/astro-ph/0703075
Appears in Collections:Publications based on data from IAO, Hanle
IIAP Publications

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