Photometry and age of star clusters in M33

Details Photometry and age of star clusters in M33 Photometry and age of star clusters in M33

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..654s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Sept. 1984, p. 654-660) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Sept.-O

Astronomy and Astrophysics

Astronomy

5

Astronomical Photometry, Electrophotometry, Spiral Galaxies, Star Clusters, Stellar Evolution, Globular Clusters, Magellanic Clouds, Stellar Color, Stellar Magnitude, Ubv Spectra

Scientific paper

Results of photoelectric UBV observations are reported for 11 star clusters in M33. The clusters of M33 are located in the same region of the two-color diagram (U-B) - (B-V) as those of the Large Magellanic Cloud. Ages of the clusters should be estimated from (0.03 - 0.1)×109 to (8 - 14)×109 years. The process of cluster formation in M33 was continuous.

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