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dc.contributor.authorDI MILLE, F.
dc.contributor.authorAlis, S.
dc.contributor.authorTAMBURINI, F.
dc.contributor.authorSaygac, Ahmet Talat
dc.contributor.authorBianchini, A.
dc.date.accessioned2021-03-05T15:12:11Z
dc.date.available2021-03-05T15:12:11Z
dc.identifier.citationBianchini A., DI MILLE F., TAMBURINI F., Saygac A. T. , Alis S., "The Slow Late Decline of the Old Nova RW Ursae Minoris (1956)", 4th International Conference on Classical and Recurrent Novae - Stella Novae: Past and Future Decades, Cape-Town, Güney Afrika, 4 - 08 Şubat 2013, cilt.490, ss.221-224
dc.identifier.othervv_1032021
dc.identifier.otherav_bac96afc-8d56-43b9-8671-762f6708555c
dc.identifier.urihttp://hdl.handle.net/20.500.12627/124227
dc.description.abstractPhotometric observations of the old nova RW UMi are presented. Data obtained mostly in the Asiago Observatory of lNAF. The period analysis of the data did not permit to recover the Retter & Lipkin (2001) period. A possible explanation to the nature of QPO in the data is given.
dc.language.isoeng
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleThe Slow Late Decline of the Old Nova RW Ursae Minoris (1956)
dc.typeBildiri
dc.contributor.departmentUniversity of Padua , ,
dc.identifier.volume490
dc.contributor.firstauthorID20801


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