UBV photometry in the nuclear bulge of the galaxy

Details UBV photometry in the nuclear bulge of the galaxy UBV photometry in the nuclear bulge of the galaxy

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....65...65l&link_type=abstract

Astronomy and Astrophysics, vol. 65, no. 1, Apr. 1978, p. 65-70. Research sponsored by the Deutsche Forschungsgemeinschaft.

Astronomy and Astrophysics

Astrophysics

2

Galactic Bulge, Galactic Nuclei, Milky Way Galaxy, Red Giant Stars, Ubv Spectra, Astronomical Photometry, Density (Number/Volume), Late Stars, Photographic Plates, Star Distribution

Scientific paper

The stellar population and its variation with increasing galactic latitude is studied for three fields with low and homogeneous absorption by UBV photometry. A comparison of color-color plots of the three fields indicates that the number of red giants decreases with increasing negative galactic latitude. The results are compared to those of McCuskey and Mehlhorn (1963) and McRae (1958).

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