Positions, magnitudes, and colors for stars in the globular cluster M15

Details Positions, magnitudes, and colors for stars in the globular cluster M15 Positions, magnitudes, and colors for stars in the globular cluster M15

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26as...51...83b&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 51, Jan. 1983, p. 83-92. Research supported by the Consiglio Nazionale delle

Astronomy and Astrophysics

Astrophysics

62

Astrometry, Globular Clusters, Star Distribution, Stellar Color, Stellar Magnitude, Stellar Spectrophotometry, Ubv Spectra, Astronomical Coordinates, Astronomical Photography, Electrophotometry, Error Analysis, Image Processing

Scientific paper

U, B, V magnitudes and positions for all the stars brighter than B = 18.6 in an annulus ranging from r = 1.9 arcmin to r = 5.0 from the center of the cluster NGC 7078 = Ml5 have been derived using a reduction method for stellar photometry in crowded fields based on a multicomponent fitting procedure applied to digitized photographic data. The accuracy of photometric and astrometric measures is discussed in detail.

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