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dc.contributor.authorPoleski, R.
dc.contributor.authorAk, Tansel
dc.contributor.authorZLOCZEWSKI, K.
dc.contributor.authorTAPPERT, C.
dc.contributor.authorEKER, ZEKİ
dc.contributor.authorRutkowski, A.
dc.contributor.authorPIETRUKOWICZ, P.
dc.contributor.authorOlech, A.
dc.date.accessioned2021-03-06T12:34:22Z
dc.date.available2021-03-06T12:34:22Z
dc.date.issued2011
dc.identifier.citationRutkowski A., PIETRUKOWICZ P., Olech A., Ak T., ZLOCZEWSKI K., Poleski R., TAPPERT C., EKER Z., "Dwarf Nova V1040 Centauri and Variable Stars in its Vicinity", ACTA ASTRONOMICA, cilt.61, ss.345-357, 2011
dc.identifier.issn0001-5237
dc.identifier.othervv_1032021
dc.identifier.otherav_f471cfc5-e5d7-49c2-b0c1-f1b57bd98b3c
dc.identifier.urihttp://hdl.handle.net/20.500.12627/160260
dc.description.abstractWe present the results of a photometric campaign of the dwarf nova V1040 Cen. The light curve shows two normal outbursts with recurrence time approximate to 40 days and amplitude approximate to 2.5 mag. Quiescence data show oscillations with periods in the range approximate to 0.1 days (2.4 h) to approximate to 0.5 days (12 h) of unknown origin. We measured the orbital period of V1040 Cen to be P(orb) = 0.060458(80) days (1.451 +/- 0.002 h). Based on the M(V)-P(orb) relation we found the distance of V1040 Cen to be 137 +/- 31 pc. In this paper we also report the detection of eleven new variable stars in the field of the monitored dwarf nova.
dc.language.isoeng
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleDwarf Nova V1040 Centauri and Variable Stars in its Vicinity
dc.typeMakale
dc.relation.journalACTA ASTRONOMICA
dc.contributor.departmentAkdeniz Üniversitesi , ,
dc.identifier.volume61
dc.identifier.issue4
dc.identifier.startpage345
dc.identifier.endpage357
dc.contributor.firstauthorID53837


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