Four-color and H-beta photometry of the galactic cluster M25

Details Four-color and H-beta photometry of the galactic cluster M25 Four-color and H-beta photometry of the galactic cluster M25

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aj.....87..650s&link_type=abstract

Astronomical Journal, vol. 87, Apr. 1982, p. 650-654.

Astronomy and Astrophysics

Astronomy

14

Cepheid Variables, Galactic Clusters, H Beta Line, Stellar Spectrophotometry, Southern Hemisphere, Stellar Luminosity

Scientific paper

Four-color and H-beta photometry has been done for 39 stars in the
galactic cluster M25. The data are used to remove nonmember stars from
the sample and to determine which stars are cluster members. A mean
distance modulus of 8.76 and color excess of E(b-y) = 0.341 is found.

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