Detection of Stars in the Dark Galactic Halo

Details Detection of Stars in the Dark Galactic Halo Detection of Stars in the Dark Galactic Halo

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..223b&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Computer Science

1

Scientific paper

The authors show how available star counts to mv = 22
together with a model of the Galaxy can be used to set limits on the
maximum brightness of the stellar constituents of a massive halo. They
find there can be few stars brighter than Mv = +14 in an
r-2 halo component.

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