- Globular Cluster formation in a collapsing supershell
Počet záznamů: 1  

Globular Cluster formation in a collapsing supershell

  1. 1.
    SYSNO ASEP0484220
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleGlobular Cluster formation in a collapsing supershell
    Author(s) Recchi, S. (IT)
    Wünsch, Richard (ASU-R) RID, ORCID
    Palouš, Jan (ASU-R) RID, ORCID
    Dinnbier, F. (CZ)
    Source TitleAstrophysics and Space Science - ISSN 0004-640X
    Roč. 362, č. 10 (2017), 10/12-10/12
    Number of pages12 s.
    Publication formPrint - P
    Languageeng - English
    CountryNL - Netherlands
    Keywordsdark age ; reionization ; first stars
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    OECD categoryAstronomy (including astrophysics,space science)
    R&D ProjectsGA15-06012S GA ČR - Czech Science Foundation (CSF)
    Institutional supportASU-R - RVO:67985815
    UT WOS000411111800002
    EID SCOPUS85028714644
    DOI https://doi.org/10.1007/s10509-017-3165-1
    AnnotationWe simulate, by means of a 1-D Eulerian hydrocode, the early evolution of the primordial cloud after the hypernova explosion, the formation of SSSs, and the following evolution, once the SSSs start to release energy and heavy elements into the interstellar medium. Our results indicate that a shell, enriched with nucleosynthetic products from SSSs, propagates inwards, towards the center of the primordial cloud. In a time span of a few Myr, this inward-propagating shell reaches a distance of only a few parsec away from the center of the primordial cloud. Its density is extremely high and its temperature very low, thus the conditions for a new episode of star formation are achieved. We study what fraction of these two distinct populations of stars can remain bound and survive until the present day. We study also under what conditions can this process repeat and form multiple stellar populations. We extensively discuss whether the proposed scenario can help to explain some open questions of the formation mechanism of globular clusters.
    WorkplaceAstronomical Institute
    ContactAnežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2018
Počet záznamů: 1  

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