Positions, magnitudes, and colors for stars in the globular cluster M92

Details Positions, magnitudes, and colors for stars in the globular cluster M92 Positions, magnitudes, and colors for stars in the globular cluster M92

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26as...53....1b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 53, July 1983, p. 1-12.

Astronomy and Astrophysics

Astrophysics

35

Astronomical Coordinates, Astronomical Photometry, Globular Clusters, Stellar Color, Stellar Magnitude, Astronomical Photography, Error Analysis

Scientific paper

B, V magnitudes and relative positions for all the stars brighter than B = 18. and V = 17.5 in an annulus ranging from r = 1.5 arcmin to r = 4.5 arcmin from the centre of the cluster NGC 6341 = M92 have been using a reduction procedure applied to digitized photographic data. Moreover, B, V magnitudes (and positions) for a second sample of stars are given in order to allow a better definition of the main branches in the Color Magnitude Diagram The accuracy of the data is discussed in detail.

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