The Photometry of Poorly Studied Open Star Clusters in the Milky Way

Details The Photometry of Poorly Studied Open Star Clusters in the Milky Way The Photometry of Poorly Studied Open Star Clusters in the Milky Way

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..934..181z&link_type=abstract

FLOWS, BOUNDARIES, INTERACTIONS: Flows, Boundaries, and Interaction Workshop. AIP Conference Proceedings, Volume 934, pp. 181-1

Computer Science

Distances, Parallaxes, Open Clusters In The Milky Way, Origin, Formation, Evolution, Age, And Star Formation, Photography And Photometry

Scientific paper

BVRI CCD photometric survey of poorly studied galactic open star clusters in the direction to Perseus spiral arm was performed with 1-meter Zeiss telescope of SAO RAS. First determinations of basic parameters for King 18 star clusters derived from original CCD BV RCIC observations are presented and compared with NIR data. The cluster has been identified as very young, with an age ~30 Myr, locating at the distance ~2.9 kpc.

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