Photographic UVBY photometry of the open cluster M52

Details Photographic UVBY photometry of the open cluster M52 Photographic UVBY photometry of the open cluster M52

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.173...69k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 173, no. 1, Nov. 1990, p. 69-76.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Photography, Open Clusters, Stellar Spectrophotometry, Ubv Spectra, B Stars, Cassiopeia Constellation, Color-Color Diagram, Hertzsprung-Russell Diagram, Interstellar Extinction

Scientific paper

Results are reported from uvby photometric observations of 15 stars in M52, obtained using the 2-m telescope of the National Astronomical Observatory of Bulgaria during October 1988 and September 1989. The data are presented in tables and graphs and used to determine characteristic stellar parameters. The distance modulus, mean reddening, and age of the cluster are found to be V0 - Mv = 11.3 + or - 0.1, E(B - V) = 0.57, and 96 Myr, respectively.

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