<?xml version="1.0" encoding="UTF-8"?>
<collection>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd http://dublincore.org/schemas/xmls/qdc/dcterms.xsd"><dc:language>eng</dc:language><dc:creator>Reisdorf, W.</dc:creator><dc:creator>Hessberger, F. P.</dc:creator><dc:creator>Kratz, J. V.</dc:creator><dc:creator>Schlitt, K.</dc:creator><dc:creator>Hildenbrand, K. D.</dc:creator><dc:creator>Hofmann, Sigurd</dc:creator><dc:creator>Münzenberg, G.</dc:creator><dc:creator>Schmidt, K.-H.</dc:creator><dc:creator>Schneider, J. H. R.</dc:creator><dc:creator>Schneider, W. F. W.</dc:creator><dc:creator>Sümmerer, K.</dc:creator><dc:creator>Wirth, G.</dc:creator><dc:title>Fusion near the threshold: A comparative study of the systems $^{40}$Ar + $^{112, 116, 122}$Sn and $^{40}$Ar + $^{144, 148, 154}$Sm</dc:title><dc:subject>info:eu-repo/classification/ddc/530</dc:subject><dc:source>Nuclear physics &amp;lt;Amsterdam&amp;gt; / A 438(1), 212 - 252 (1985). doi:10.1016/0375-9474(85)90125-3</dc:source><dc:type>info:eu-repo/semantics/article</dc:type><dc:type>info:eu-repo/semantics/publishedVersion</dc:type><dc:publisher>North-Holland Publ. Co.</dc:publisher><dc:date>1985</dc:date><dc:rights>info:eu-repo/semantics/closedAccess</dc:rights><dc:coverage>DE</dc:coverage><dc:identifier>https://repository.gsi.de/record/218961</dc:identifier><dc:identifier>https://repository.gsi.de/search?p=id:%22GSI-2019-00767%22</dc:identifier><dc:audience>Researchers</dc:audience><dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1016/0375-9474(85)90125-3</dc:relation><dc:relation>info:eu-repo/semantics/altIdentifier/issn/0375-9474</dc:relation><dc:relation>info:eu-repo/semantics/altIdentifier/issn/1873-1554</dc:relation><dc:relation>info:eu-repo/semantics/altIdentifier/wos/WOS:A1985AGW3300011</dc:relation></oai_dc:dc>

</collection>