Integrated parameters of open clusters

Details Integrated parameters of open clusters Integrated parameters of open clusters

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.236..263p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 236, Jan. 1, 1989, p. 263-276.

Astronomy and Astrophysics

Astronomy

27

Open Clusters, Star Clusters, Magellanic Clouds, Milky Way Galaxy, Stellar Color, Stellar Magnitude

Scientific paper

Integrated magnitudes and colors of population I synthetic clusters have been derived using theoretical evolutionary tracks and an age-dependednt initial mass function. A comparison of the theoretically obtained integrated parameters with the observational data of open clusters in the Milky Way and clusters in the LMC has also been made. It is found that the observed dependences show a better agreement with the theoretical dependences obtained in the present work than the theoretical dependences obtained by earlier authors. It is also concluded that the clusters in the LMC in general show a mean reddening of E(B-V) = 0.12 mag.

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