{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2022,3,29]],"date-time":"2022-03-29T03:28:07Z","timestamp":1648524487725},"reference-count":5,"publisher":"Cambridge University Press (CUP)","issue":"S304","license":[{"start":{"date-parts":[[2014,7,25]],"date-time":"2014-07-25T00:00:00Z","timestamp":1406246400000},"content-version":"unspecified","delay-in-days":297,"URL":"https:\/\/www.cambridge.org\/core\/terms"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Proc. IAU"],"published-print":{"date-parts":[[2013,10]]},"abstract":"<jats:title>Abstract<\/jats:title><jats:p>Physical conditions and oxygen and nitrogen abundances in 36 SBS UV-excess and\/or emission-line galaxies from the SDSS DR7 were determined. We have found that SBS 0808+578 is AGN. The others are HII galaxies or HII regions in galaxies. For all objects the oxygen abundance 12+log(O\/H) lies in the range of 7.85 \u00f7 8.61 and log(N\/O) ratio in the range of \u22121.45 \u00f7 \u22120.4. They occupy the same area in the diagram N\/O O\/H as the high-excitation HII regions. We found no extremely metal-deficient galaxy. Using H-alpha fluxes star formation rates (SFR) for our samples galaxies were determined. Determined SFRs, being in the range of 0.001 \u00f7 6 o year<jats:sup>\u22121<\/jats:sup>, are similar of that observed in typical star forming regions in spiral and irregular galaxies.<\/jats:p>","DOI":"10.1017\/s1743921314003226","type":"journal-article","created":{"date-parts":[[2014,7,25]],"date-time":"2014-07-25T10:59:50Z","timestamp":1406285990000},"page":"34-35","source":"Crossref","is-referenced-by-count":0,"title":["The physical conditions and oxygen and nitrogen abundance of 36 SBS galaxies from the SDSS DR7"],"prefix":"10.1017","volume":"9","author":[{"given":"M. V.","family":"Gyulzadyan","sequence":"first","affiliation":[]},{"given":"V. Z.","family":"Adibekyan","sequence":"additional","affiliation":[]}],"member":"56","published-online":{"date-parts":[[2014,7,25]]},"reference":[{"key":"S1743921314003226_ref1","first-page":"87","volume":"415","author":"Izotov","year":"2004","journal-title":"AandA"},{"key":"S1743921314003226_ref3","first-page":"874","volume":"354","author":"Pilyugin","year":"2000","journal-title":"AandA"},{"key":"S1743921314003226_ref2","first-page":"955","volume":"448","author":"Izotov","year":"2006","journal-title":"AandA"},{"key":"S1743921314003226_ref4","first-page":"L127","volume":"454","author":"Stasiska","year":"2006","journal-title":"AandA"},{"key":"S1743921314003226_ref5","first-page":"155","volume":"41","author":"Stepanyan","year":"2005","journal-title":"Rev. Mexicana AyA"}],"container-title":["Proceedings of the International Astronomical Union"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.cambridge.org\/core\/services\/aop-cambridge-core\/content\/view\/S1743921314003226","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2019,4,23]],"date-time":"2019-04-23T19:55:50Z","timestamp":1556049350000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.cambridge.org\/core\/product\/identifier\/S1743921314003226\/type\/journal_article"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2013,10]]},"references-count":5,"journal-issue":{"issue":"S304","published-print":{"date-parts":[[2013,10]]}},"alternative-id":["S1743921314003226"],"URL":"https:\/\/doi.org\/10.1017\/s1743921314003226","relation":{},"ISSN":["1743-9213","1743-9221"],"issn-type":[{"value":"1743-9213","type":"print"},{"value":"1743-9221","type":"electronic"}],"subject":[],"published":{"date-parts":[[2013,10]]}}}