Interstellar reddening in the direction of the globular cluster M71

Details Interstellar reddening in the direction of the globular cluster M71 Interstellar reddening in the direction of the globular cluster M71

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.100...95j&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 100, no. 1-2, March 1984, p. 95-106.

Astronomy and Astrophysics

Astrophysics

12

Astronomical Photometry, Globular Clusters, Interstellar Extinction, Star Clusters, Astronomical Catalogs, Star Distribution, Stellar Color

Scientific paper

Interstellar reddening as a function of distance in the direction of the globular cluster M71 is determined by two-dimensional quantification of 96 foreground stars observed in the Vilnius photometric system. In concentric areas with the radii 30arcmin and 10arcmin centered on the cluster the reddening shows the same variations ranging from EB-V = 0.12 to 0.32. The cluster stars are likely to have variable extinction too, at least in the outer regions of the cluster.

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