Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-13T05:54:37.550Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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