A photoelectric UBV sequence in SA 184

Details A photoelectric UBV sequence in SA 184 A photoelectric UBV sequence in SA 184

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...67..103a&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 67, no. 1, Jan. 1987, p. 103-110.

Astronomy and Astrophysics

Astrophysics

9

Electrophotometry, Milky Way Galaxy, Stellar Spectrophotometry, Ubv Spectra, Astronomical Coordinates, Magellanic Clouds, Star Distribution

Scientific paper

A photometric sequence in SA 184 is presented. A total of 135 UBV observations have been made for 27 sequence stars. They range in B from 7.1 to 20.2 and in B-V from +0.2 to +1.6. The resulting accuracy of magnitudes and colours should internally as well as externally be around or better than 0.02 magnitude for most of the data presented. Accurate coordinates are given together with identification maps. The resulting UBV data are plotted in a two-colour diagram. Some results are discussed.

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