<Record><identifier xmlns="http://purl.org/dc/elements/1.1/">URN:NBN:SI:doc-HA5HNXRB</identifier><date>2023</date><creator>Jamnik, Bor</creator><relation>documents/doc/H/URN_NBN_SI_doc-HA5HNXRB_001.pdf</relation><relation>documents/doc/H/URN_NBN_SI_doc-HA5HNXRB_001.txt</relation><format format_type="issue">1</format><format format_type="volume">10</format><format format_type="extent">8 str.</format><format format_type="type">article</format><identifier identifier_type="COBISSID_HOST">150836995</identifier><identifier identifier_type="ISSN">2385-8567</identifier><identifier identifier_type="URN">URN:NBN:SI:doc-HA5HNXRB</identifier><language>eng</language><publisher publisher_location="Ljubljana">Založba Fakultete za matematiko in fiziko Univerze v Ljubljani</publisher><source>Matrika</source><rights>InC</rights><subject language_type_id="slv">astrofizika</subject><subject language_type_id="eng">astrophysics</subject><subject language_type_id="eng">binary stars</subject><subject language_type_id="eng">chemical homogeneity</subject><subject language_type_id="slv">dvojne zvezde</subject><subject language_type_id="eng">galactic archaeology</subject><subject language_type_id="slv">galaktična arheologija</subject><subject language_type_id="slv">kemijska homogenost</subject><title>The limits of chemical homogeneity - the case of binary stars</title></Record>