{BOAO Photometric Survey of Galactic Open Clusters. II. Physical Parameters of 12 Open Clusters
arXiv:astro-ph/0203028 · doi:10.1086/338309
Abstract
We have initiated a long-term project, the BOAO photometric survey of open clusters, to enlarge our understanding of galactic structure using UBVI CCD photometry of open clusters which have been little studied before. This is the second paper of the project in which we present the photometry of 12 open clusters. We have determined the cluster parameters by fitting the Padova isochrones to the color-magnitude diagrams of the clusters. All the clusters except for Be 0 and NGC 1348 are found to be intermediate-age to old (0.2 - 4.0 Gyrs) open clusters with a mean metallicity of [Fe/H] = 0.0.
11 pages
Cited by in corpus (18)
- On the Galactic Disk Metallicity Distribution from Open Clusters I. New Catalogues and Abundance Gradient
- Analysing the database for stars in open clusters I. General methods and description of the data
- Overlapping abundance gradients and azimuthal gradients related to the spiral structure of the Galaxy
- Sejong Open Cluster Survey (SOS). 0. Target Selection and Data Analysis
- On the recent star formation history of the Milky Way disk
- On the metallicity of open clusters I. Photometry
- The Swift/UVOT Stars Survey. III. Photometry and Color-Magnitude Diagrams of 103 Galactic Open Clusters
- Radial velocities and metallicities from infrared Ca II triplet spectroscopy of open clusters: Berkeley 26, Berkeley 70, NGC 1798, and NGC 2266
- Photometric and Kinematic study of the three intermediate age open clusters NGC 381, NGC 2360, and Berkeley 68
- Three new bricks in the wall: Berkeley 23, Berkeley 31, and King 8
- Blue Straggler Stars in Galactic Open Clusters and the effect of field star contamination
- Exploring FSR open cluster candidates within of the Galactic anticentre
- CCD Photometry of Twenty Open Clusters
- Understanding the Planetary Formation and Evolution in Star Clusters(UPiC)-I: Evidence of Hot Giant Exoplanets Formation Timescales
- Radial velocities and metallicities from infrared Ca II triplet spectroscopy of open clusters II. Berkeley 23, King 1, NGC 559, NGC 6603 and NGC 7245
- Open Clusters as Probes of the Galactic Magnetic Field: I. Cluster Properties
- BOAO Photometric Survey of Galactic Open Clusters. III. Czernik 24 and Czernik 27
- A Photometric Study of Five Open Clusters in the SDSS