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Observational manifestations of sequential star formation in giant star-gas complexes of the Galaxy

Published online by Cambridge University Press:  03 August 2017

T. G. Sitnik
T. G. Sitnik*
Affiliation:
Sternberg Astronomical Institute, 13 Universitetskij prospect, Moscow V-234, 119899, USSR

Abstract

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The age distribution of stars and stellar groupings was studied in the galactic large-scale star-gas complexes (SGCs).

Type
Large Scale Structure
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 21 - 24
Copyright
Copyright © Kluwer 1991 

References

1. Efremov, Yu. N., Sitnik, (1988). Soviet. Astron. Letters 14, 347.Google Scholar
2. Sitnik, T. G. (1989). Pisma v Astron. Zh. 15. 897.Google Scholar
3. Sitnik, T. G. (1991). Pisma v Astron. Zh. to be published.Google Scholar
4. Maeder, A. (1981). Astron. Astrophys. 102, 401; (1983), 120, 113.Google Scholar
5. Efremov, Yu. N. (1989). Stellar complexes. Astrophys. Space Sci. Rev. 7.Google Scholar
6. Mermilliod, J. C. (1981). Astron. Astrophys. 97, 235.Google Scholar
7. Efremov, Yu. N. (1978). Soviet Astron. Letters 4, 66; (1979), 5 12.Google Scholar
8. Ellmegreen, B. G., Elmegreen, D. M. (1983). Month. Notic. Roy. Astron. Soc. 203, 31.Google Scholar