<Record><identifier xmlns="http://purl.org/dc/elements/1.1/">URN:NBN:SI:doc-2XVDY9UO</identifier><date>2012</date><creator>Haensel, Pawel</creator><creator>Rosina, Mitja</creator><creator>Soni, Vikram</creator><relation>documents/doc/2/URN_NBN_SI_doc-2XVDY9UO_001.pdf</relation><relation>documents/doc/2/URN_NBN_SI_doc-2XVDY9UO_001.txt</relation><format format_type="issue">1</format><format format_type="volume">13</format><format format_type="type">article</format><format format_type="extent">str. 42-46</format><identifier identifier_type="ISSN">1580-4992</identifier><identifier identifier_type="COBISSID">26281255</identifier><identifier identifier_type="URN">URN:NBN:SI:doc-2XVDY9UO</identifier><language>eng</language><publisher publisher_location="Ljubljana">DMFA - založništvo</publisher><source>Blejske delavnice iz fizike</source><rights>InC</rights><subject language_type_id="slv">astrofizika</subject><subject language_type_id="slv">fizika elementarnih delcev</subject><subject language_type_id="slv">jedrska fizika</subject><title>The implications of the two solar mass neutron star for the strong interactions</title></Record>