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Study of nova shells .2. FH Serentis 1970 and QU Vulpeculae 1984, nebular expansion, parallax and luminosity

dc.contributor.authorGilmozzi, Roberto
dc.contributor.authorEsenoglu, Hasan Hüseyin
dc.contributor.authorBianchini, Antonio
dc.contributor.authorDella Valle, Massimo
dc.date.accessioned2021-03-03T19:47:51Z
dc.date.available2021-03-03T19:47:51Z
dc.date.issued1997
dc.identifier.citationDella Valle M., Gilmozzi R., Bianchini A., Esenoglu H. H. , "Study of nova shells .2. FH Serentis 1970 and QU Vulpeculae 1984, nebular expansion, parallax and luminosity", ASTRONOMY & ASTROPHYSICS, cilt.325, sa.3, ss.1151-1156, 1997
dc.identifier.issn0004-6361
dc.identifier.othervv_1032021
dc.identifier.otherav_567672e5-ff5e-42ce-9a0b-3978dc751603
dc.identifier.urihttp://hdl.handle.net/20.500.12627/61048
dc.description.abstractWe present H alpha direct imaging and shell spectroscopic observations of two classical novae: FH Ser 1970 and QU Vul 1984. The distances, reddenings, luminosities at maximum, and the mass of the shell ejected by FH Ser are derived and discussed.
dc.language.isoeng
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleStudy of nova shells .2. FH Serentis 1970 and QU Vulpeculae 1984, nebular expansion, parallax and luminosity
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS
dc.contributor.department, ,
dc.identifier.volume325
dc.identifier.issue3
dc.identifier.startpage1151
dc.identifier.endpage1156
dc.contributor.firstauthorID40517


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