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Star complexes and starburst clumps in spiral galaxies

2004/10/28 by Yu. N. Efremov, Efremov, Yu. N.
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0410702

Contribution to the Transactions of the conference "Gamov-100", Odessa, August 2004

arxiv created 2004/10/28 · openalex publication_date 2004/10/28 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Star complexes are the highest level groupings in the hierarchy of the embedded young stars, clusters and associations, which obey the size - age relation. Starburst clumps, superassociations, supergiant HII regions are different titles for the groupings of the same size as complexes but with active star formation over all the grouping. The coherent star formation in the regions of violent star formation was probably triggered by external pressure. The issue of gravitational boundness of complexes and superassociations is briefly discussed

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