Interstellar reddening in the direction of the globular cluster M15

Details Interstellar reddening in the direction of the globular cluster M15 Interstellar reddening in the direction of the globular cluster M15

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992balta...1...25j&link_type=abstract

Baltic Astronomy, vol. 1, p. 25

Astronomy and Astrophysics

Astronomy

4

Interstellar Extinction, Globular Clusters, Open Clusters, Error Analysis, Peculiar Stars, Binary Stars

Scientific paper

Interstellar reddening as a function of distance in the direction of the globular cluster M15 is determined using two-dimensional quantification of 77 foreground stars in the Vilnius photometric system. The observed average value of AV calculated for the stars, which are farther than the expected edge of the absorbing dust layer, is 0.26 +/- 0.02. This is in good agreement with the AV determined from the cluster integrated B-V color index.

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