Photoelectric UBVRI sequences in the sculptor group galaxies NGC 45, NGC 55, NGC 247, NGC 253, NGC 300, and NGC 7793

Details Photoelectric UBVRI sequences in the sculptor group galaxies NGC 45, NGC 55, NGC 247, NGC 253, NGC 300, and NGC 7793 Photoelectric UBVRI sequences in the sculptor group galaxies NGC 45, NGC 55, NGC 247, NGC 253, NGC 300, and NGC 7793

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89..814a&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 89, June 1984, p. 814-818.

Other

7

Astronomical Spectroscopy, Electrophotometry, Galactic Clusters, Ubv Spectra, Astrometry, Astronomical Catalogs, Galactic Radiation, Magnitude, Spiral Galaxies

Scientific paper

NGC 45, 55, 247, 253, 300, and 7793, are the conspicuous Sculptor Group
galaxies for which photoelectric UBVRI sequences have been set up. The
purpose of these sequences is to provide direct, zero-point calibrations
for the study of the brighter stars, and, by means of a Pickering-Racine
prism, CCD, or other photometric device, stars of fainter magnitude.

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