<Record><identifier xmlns="http://purl.org/dc/elements/1.1/">URN:NBN:SI:DOC-K1WQYXKB</identifier><date>1883</date><creator>Vodušek, Matej</creator><relation>documents/doc/K/urn_nbn_si_doc-k1wqyxkb_001.pdf</relation><relation>documents/doc/K/urn_nbn_si_doc-k1wqyxkb_001.txt</relation><relation>documents/doc/K/urn_nbn_si_doc-k1wqyxkb_001.xml</relation><format format_type="main">176 str.</format><format format_type="extent">V, 162, 28 str., 23 cm</format><identifier identifier_type="COBISSID">87965696</identifier><identifier identifier_type="URN">urn:nbn:si:doc-k1wqyxkb</identifier><language>ger</language><publisher>I. v. Kleinmayr &amp; F. Bamberg</publisher><source>knjige</source><rights>PDM</rights><subject language_type_id="   ">astronomija</subject><subject language_type_id="   ">določevanje</subject><subject language_type_id="   ">kometi</subject><subject language_type_id="   ">lunina paralaksa</subject><subject language_type_id="   ">metode</subject><subject language_type_id="   ">planeti</subject><subject language_type_id="   ">sončna paralaksa</subject><subject language_type_id="   ">tirnice</subject><title>Neue exacte Methode für die Bahnbestimmung der Planeten und Kometen nebst einer neuen Störungstheorie</title></Record>