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CCD Washington photometry of three highly field star contaminated open clusters in the third Galactic quadrant

Authors :
M. C. Parisi
Andrea Veronica Ahumada
Andrés E. Piatti
Juan J. Clariá
Source :
New Astronomy. 14:97-108
Publication Year :
2009
Publisher :
Elsevier BV, 2009.

Abstract

We present CCD photometry in the Washington system C and T1 passbands down to T1 ~ 19.5 mag in the fields of Czernik 26, Czernik 30, and Haffner 11, three poorly studied open clusters located in the third Galactic quadrant. We measured T1 magnitudes and C-T1 colors for a total of 6472 stars distributed throughout cluster areas of 13.6´ x 13.6´ each. Cluster radii were estimated from star counts in appropriate-sized boxes distributed throughout the entire observed fields. Based on the best fits of isochrones computed by the Padova group to the (C-T_1,T_1) color-magnitude diagrams (CMDs), we derived color excesses, heliocentric distances and ages for the three clusters. These are characterized by a relatively small angular size and by a high field star contamination. We performed a firm analysis of the field star contamination of the CMDs and examined different relationships between the position in the Galaxy of known open clusters located within 1 kpc around the three studied ones, their age and their interstellar visual absorption. We confirm previous results in the sense that the closer the cluster birthplace to the Galactic plane, the higher the interstellar visual absorption. We also found that the space velocity dispersion perpendicular to the Galactic plane diminishes as the clusters are younger. The positions, interstellar visual absorptions,ages, and metallicities of the three studied clusters favor the hypothesis that they were not born in the recently discovered Canis Major (CMa) dwarf galaxy before it was accreted by the Milky Way. Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Parisi, Maria Celeste. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Ahumada, Andrea Veronica. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina

Details

ISSN :
13841076
Volume :
14
Database :
OpenAIRE
Journal :
New Astronomy
Accession number :
edsair.doi.dedup.....dba04e7ff0dd48d8c3f25c9a00c52738
Full Text :
https://doi.org/10.1016/j.newast.2008.05.006