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The re-analysis of the ROSAT data of Nova Mus 1983 using white dwarf atmosphere emission models

dc.contributor.authorBalman, Şölen
dc.contributor.authorKrautter, J.
dc.date.accessioned2021-03-02T22:32:43Z
dc.date.available2021-03-02T22:32:43Z
dc.date.issued2001
dc.identifier.citationBalman Ş., Krautter J., "The re-analysis of the ROSAT data of Nova Mus 1983 using white dwarf atmosphere emission models", Monthly Notices of the Royal Astronomical Society, cilt.326, sa.4, ss.1441-1447, 2001
dc.identifier.issn0035-8711
dc.identifier.othervv_1032021
dc.identifier.otherav_0d3cebf3-e12f-4a7b-bcc8-a9f942312547
dc.identifier.urihttp://hdl.handle.net/20.500.12627/14517
dc.identifier.urihttps://doi.org/10.1111/j.1365-2966.2001.04716.x
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=0010994620&origin=inward
dc.language.isoeng
dc.titleThe re-analysis of the ROSAT data of Nova Mus 1983 using white dwarf atmosphere emission models
dc.typeMakale
dc.relation.journalMonthly Notices of the Royal Astronomical Society
dc.contributor.departmentOrta Doğu Teknik Üniversitesi , ,
dc.identifier.volume326
dc.identifier.issue4
dc.identifier.startpage1441
dc.identifier.endpage1447
dc.contributor.firstauthorID2212672


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