RGU-photometric space-densities in a field close to NGC 7006 compared with the gradients predicted by the 5 Basle standard models

Details RGU-photometric space-densities in a field close to NGC 7006 compared with the gradients predicted by the 5 Basle standard models RGU-photometric space-densities in a field close to NGC 7006 compared with the gradients predicted by the 5 Basle standard models

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...88..233f&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 88, no. 2, May 1991, p. 233-244. SNSF-supported research.

Astronomy and Astrophysics

Astrophysics

2

Astronomical Models, Astronomical Photometry, Galactic Structure, Main Sequence Stars, Space Density, Density Distribution, Synoptic Measurement

Scientific paper

Results are presented of the third contribution of the postsynopsis section to the Model Comparison Phase (MCP) of the Basle Halo Program, in which three-color (RGU) photometrically determined (Fenkart et al., 1987) total space density histograms for late-type giants and 1-m-interval main sequence M(G) groups, with M(G) between 5 m and 8 m, along the direction to NGC 7006 were compared with gradients predicted by the set of five Basle standard models of the MCP. Results obtained from histograms of late-type giants strongly support the prediction of a Thick Disk component in the direction to NGC 7006 and results for the main-sequence group do not contradict the Thick-Disk prediction.

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