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The astrophysical consequences of the bimodal hydrodynamic solution of the super star cluster winds
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SYSNO ASEP 0335818 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title The astrophysical consequences of the bimodal hydrodynamic solution of the super star cluster winds Title Astrofyzikální důsledky bimodálního hydrodynamického řešení větrů super-hvězdokup Author(s) Palouš, Jan (ASU-R) RID, ORCID
Wünsch, Richard (ASU-R) RID, ORCID
Tenorio-Tagle, G. (MX)
Silich, S. (MX)Source Title Astrophysics and Space Science - ISSN 0004-640X
Roč. 324, 2-4 (2009), s. 195-198Number of pages 4 s. Language eng - English Country NL - Netherlands Keywords stellar winds ; star clusters ; HII regions Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects LC06014 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000272018700020 DOI 10.1007/s10509-009-0127-2 Annotation In bimodal regime, the inner part of the cluster is unstable, while in the outer the out-blowing wind is formed. We show consequences of this solution to the galactic superwinds and discuss its open issues. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2010
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