The Old-Nova Gk Per .2. Optical Outbursts

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dc.contributor.authorBianchini, A
dc.contributor.authorSabbadin, F
dc.contributor.authorHamzaoglu, E
dc.date.accessioned2019-10-27T11:38:03Z
dc.date.available2019-10-27T11:38:03Z
dc.date.issued1982
dc.departmentEge Üniversitesien_US
dc.identifier.endpage178en_US
dc.identifier.issn0004-6361
dc.identifier.issue1en_US
dc.identifier.startpage176en_US
dc.identifier.urihttps://hdl.handle.net/11454/34243
dc.identifier.volume106en_US
dc.identifier.wosWOS:A1982NC04800035en_US
dc.identifier.wosqualityN/Aen_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.language.isoenen_US
dc.publisherEdp Sciences S Aen_US
dc.relation.ispartofAstronomy & Astrophysicsen_US
dc.relation.publicationcategoryDiğeren_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.titleThe Old-Nova Gk Per .2. Optical Outburstsen_US
dc.typeOtheren_US

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