RGU three-colour photometric parameters of the galactic cluster CR 299

Details RGU three-colour photometric parameters of the galactic cluster CR 299 RGU three-colour photometric parameters of the galactic cluster CR 299

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26as...56...11t&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 56, April 1984, p. 11-15. Research supported by the Swiss Na

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, Colorimetry, Star Clusters, Galactic Structure, Photographic Plates, Stellar Color, Stellar Magnitude, Visual Photometry

Scientific paper

The three-color photometric method A, first presented by Becker (1963), is presently used to obtain the photometrically determinable parameters of the galactic cluster Cr 299. The apparent concentrations in the SW and SE areas of the region studied are noted to not be photometrically physical, while for Cr 299 the reddening, absorption, distance, probable physical members and earliest spectral type could be evaluated.

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