Galaxies and Stars

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Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003arep...47..531f&link_type=abstract

Astronomy Reports, vol. 47, Issue 7, p.531-534

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The distribution of galaxies in the vicinity of stars brighter than V=7.25m is analyzed. The number density of galaxies is slightly decreased in such regions. This result is statistically significant and cannot be explained as a direct effect of the extended photographic images of these stars. The result is apparently associated with the presence of clouds near the stars, which absorb or scatter light.

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