Four-color and H-beta photometry of stars in NGC 7654 and M25

Details Four-color and H-beta photometry of stars in NGC 7654 and M25 Four-color and H-beta photometry of stars in NGC 7654 and M25

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pasp...89..546s&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 89, Aug.-Sept. 1977, p. 546-549.

Astronomy and Astrophysics

Astronomy

13

Cepheid Variables, H Beta Line, Star Clusters, Stellar Spectrophotometry, Ubv Spectra, Optical Properties, Stellar Luminosity

Scientific paper

Four-color and H-beta photometry has been obtained of stars in the
galactic clusters NGC 7654 and M25. An analysis of these data shows
variable extinction in both clusters. The distance modulus of NGC 7654
is found to be 10.99 plus or minus 0.2 and that of M25 is 8.68 plus or
minus 0.1.

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