Comparisons of the Standard Galaxy Model with observations in two fields

Details Comparisons of the Standard Galaxy Model with observations in two fields Comparisons of the Standard Galaxy Model with observations in two fields

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.213p..39b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 213, March 15, 1985, p. 39P-41P.

Astronomy and Astrophysics

Astronomy

12

Astronomical Models, Milky Way Galaxy, Star Distribution, Globular Clusters, Stellar Color, Stellar Luminosity

Scientific paper

The Bahcall-Soneira (1984) model for the distribution of stars in the Galaxy is compared with the observations reported by Gilmore, Reid, and Hewett (1984) in two directions in the sky, the pole and the Morton-Tritton (1982) region. It is shown that the Galaxy model is in good agreement with the observations everywhere it has been tested with modern data, including the magnitude range, V = 17-18, and provided that the globular cluster feature is included in the luminosity function of the field Population II stars.

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