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Extragalactic star-forming regions and open clusters in the Milky Way

Published online by Cambridge University Press:  18 January 2010

F. Sakhibov ,
A. S. Gusev ,
N. V. Kharchenko  and
A. E. Piskunov
F. Sakhibov
Affiliation:
Giessen–Friedberg University for Applied Sciences, Friedberg, Germany Institute of Astrophysics, Academy of Sciences of Tajikistan, Dushanbe, Tajikistan
A. S. Gusev
Affiliation:
Sternberg Astronomical Institute, Moscow, Russia
N. V. Kharchenko
Affiliation:
Main Astronomical Observatory National Academy of Sciences of Ukraine, Kiev, Ukraine
A. E. Piskunov
Affiliation:
Institute of Astronomy of the Russian Academy of Sciences, Moscow, Russia
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Abstract

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We have carried out a comparative analysis of the evolution of integrated photometric parameters of young star-forming complexes in spiral and irregular galaxies and Galactic open clusters. We find that when the interstellar extinction is properly taken into account, the extragalactic complexes observed as giant Hii regions and open clusters in the Milky Way form a single evolutionary sequence of objects evolving at different stages.

Keywords

open clusters and associations: generalgalaxies: star clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S266: Star clusters: basic galactic building blocks throughout time and space , August 2009 , pp. 522
Copyright
Copyright © International Astronomical Union 2010