{"?xml":{"@version":"1.0"},"edm:RDF":{"@xmlns:dc":"http://purl.org/dc/elements/1.1/","@xmlns:edm":"http://www.europeana.eu/schemas/edm/","@xmlns:wgs84_pos":"http://www.w3.org/2003/01/geo/wgs84_pos","@xmlns:foaf":"http://xmlns.com/foaf/0.1/","@xmlns:rdaGr2":"http://rdvocab.info/ElementsGr2","@xmlns:oai":"http://www.openarchives.org/OAI/2.0/","@xmlns:owl":"http://www.w3.org/2002/07/owl#","@xmlns:rdf":"http://www.w3.org/1999/02/22-rdf-syntax-ns#","@xmlns:ore":"http://www.openarchives.org/ore/terms/","@xmlns:skos":"http://www.w3.org/2004/02/skos/core#","@xmlns:dcterms":"http://purl.org/dc/terms/","edm:WebResource":[{"@rdf:about":"http://www.dlib.si/stream/URN:NBN:SI:doc-AX6G6L0F/344664232d71bc3f-41042d6dc---c0af94a/PDF","dcterms:extent":"1992 KB"},{"@rdf:about":"http://www.dlib.si/stream/URN:NBN:SI:doc-AX6G6L0F/4404d49d-6d23-46c3-a1c3-a67c04f1bf22/TEXT","dcterms:extent":"19 KB"}],"edm:TimeSpan":{"@rdf:about":"2014-2024","edm:begin":{"@xml:lang":"en","#text":"2014"},"edm:end":{"@xml:lang":"en","#text":"2024"}},"edm:ProvidedCHO":{"@rdf:about":"URN:NBN:SI:doc-AX6G6L0F","dcterms:isPartOf":[{"@rdf:resource":"https://www.dlib.si/details/URN:NBN:SI:spr-OE00UKYR"},{"@xml:lang":"sl","#text":"Matrika"}],"dcterms:issued":"2021","dc:creator":"Perko, Manica","dc:format":[{"@xml:lang":"sl","#text":"številka:1"},{"@xml:lang":"sl","#text":"7 str."},{"@xml:lang":"sl","#text":"letnik:8"}],"dc:identifier":["ISSN:2385-8567","COBISSID_HOST:59111171","URN:URN:NBN:SI:doc-AX6G6L0F"],"dc:language":"en","dc:publisher":{"@xml:lang":"sl","#text":"Založba Fakultete za matematiko in fiziko Univerze v Ljubljani"},"dc:subject":[{"@xml:lang":"sl","#text":"binarni sistemi"},{"@xml:lang":"en","#text":"binary systems"},{"@xml:lang":"en","#text":"stars"},{"@xml:lang":"sl","#text":"zvezde"}],"dcterms:temporal":{"@rdf:resource":"2014-2024"},"dc:title":{"@xml:lang":"sl","#text":"X-ray binary stars|"},"dc:description":[{"@xml:lang":"sl","#text":"A binary system is a system that contains two stars which orbit around the center of mass of the system. In an X-ray binary systems one of the two stars is a very small and dense object called a neutron star. A neutron star is a collapsed core of a star which had a mass of more than 8 solar masses. The mass transfer in a high-mass X-ray binary is driven by strong stellar winds and in a low-mass X-ray binary the mass is transferred via Roche lobe overflow"},{"@xml:lang":"sl","#text":"Dvojni sistemi zvezd vsebujejo dve zvezdi, ki krožita okrog skupnega masnega središča. V rentgenskih dvojnih sistemih je ena izmed zvezd zelo gost in majhen objekt, nevtronska zvezda. Nevtronska zvezda je ostanek jedra zvezde, ki je imela maso večjo od 8 sončevih mas. Prenos mase v rentgenskih dvojnih sistemih z veliko maso poteka zaradi močnih zvezdnih vetrov. V dvojnih sistemih z majhno maso pa se material prenaša preko Rochovega ovala"}],"edm:type":"TEXT","dc:type":[{"@xml:lang":"sl","#text":"znanstveno časopisje"},{"@xml:lang":"en","#text":"journals"},{"@rdf:resource":"http://www.wikidata.org/entity/Q361785"}]},"ore:Aggregation":{"@rdf:about":"http://www.dlib.si/?URN=URN:NBN:SI:doc-AX6G6L0F","edm:aggregatedCHO":{"@rdf:resource":"URN:NBN:SI:doc-AX6G6L0F"},"edm:isShownBy":{"@rdf:resource":"http://www.dlib.si/stream/URN:NBN:SI:doc-AX6G6L0F/344664232d71bc3f-41042d6dc---c0af94a/PDF"},"edm:rights":{"@rdf:resource":"http://rightsstatements.org/vocab/InC/1.0/"},"edm:provider":"Slovenian National E-content Aggregator","edm:dataProvider":{"@xml:lang":"en","#text":"National and University Library of Slovenia"},"edm:object":{"@rdf:resource":"http://www.dlib.si/streamdb/URN:NBN:SI:doc-AX6G6L0F/maxi/edm"},"edm:isShownAt":{"@rdf:resource":"http://www.dlib.si/details/URN:NBN:SI:doc-AX6G6L0F"}}}}