Distribution of Astrometric Binaries in Various Galactic Latitudes

Details Distribution of Astrometric Binaries in Various Galactic Latitudes Distribution of Astrometric Binaries in Various Galactic Latitudes

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.110..125g&link_type=abstract

Astrophysics and Space Science, Volume 110, Issue 1, pp.125-131

Astronomy and Astrophysics

Astrophysics

Scientific paper

The conclusions of the present paper broadly are: (a) The galactic concentration of doubles by comparing the distributions in galactic latitudes 0°<β≤20° and β>40° is nearly twice as large as the galactic concentration of stars in general. (b) The astrographic catalogues are not complete in the fainter magnitudes. (c) The large value of the ratioT:O k (observed to optical number of pairs) from Kreiken's formula shows that almost all stars in the group 0″

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