Integrated Photometry of open clusters (Battinelli+ 1994)

Details Integrated Photometry of open clusters (Battinelli+ 1994) Integrated Photometry of open clusters (Battinelli+ 1994)

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ycat..41040379b&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/104/379. Originally published in: 1994A&AS..104..379B

Statistics

Methodology

Clusters: Open, Photometry

Scientific paper

Galactic open clusters provide an abundant sample of stellar aggregates of various sizes, ages and metal abundances, apt to constitute a template for comparison with star systems in other galaxies. In this paper we present and discuss a standard methodology to synthesize U,B,V fluxes and colours, and apply it to a set of 138 open clusters. Results are compared with previous ones available in the literature. We were able to calibrate a mass-luminosity relation by which we evaluated the mass of ~ 400 open clusters, leading to a well defined present-day mass function. The number-complete sample of galactic open clusters presented in Battinelli & Capuzzo-Dolcetta (1992AJ....103.1596B) is enlarged of a 15%. (3 data files).

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