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Turkish Journal of Physics

DOI

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Abstract

A low-latitude anticenter field (l = 189°, b = +21°) is investigated by using the full calibration tools of RGU photometry. The observed RGU data are reduced to the standard system and the separation of dwarfs and evolved stars is carried out by an empirical method. Stars are categorized into three metallicity classes, i.e. -0.25

Keywords

Galaxy: structure -- Stars: luminosity function -- Photometry: RGU.

First Page

289

Last Page

299

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