RGU three-colour photometry of a starfield in anticentre-direction (A6)

Details RGU three-colour photometry of a starfield in anticentre-direction (A6) RGU three-colour photometry of a starfield in anticentre-direction (A6)

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...59...73f&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 59, Jan. 1985, p. 73-81. Research supported by the Swiss Nat

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, Galactic Structure, Star Distribution, Interstellar Extinction, Space Density, Stellar Luminosity

Scientific paper

The reddening, density, and luminosity functions determined for 1362 stars in a field of 0.217 sq deg, in the anticenter direction, are compared with the corresponding results in another anticenter field which lies only about 7 deg apart from it. While the character of the overall density function is not significantly different in both fields, those of limited M(G) intervals, as well as the individual absorption situations, can differ considerably even between those observing directions that lie only a few degrees apart.

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