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ON THE FURTHER OBSERVATIONS OF B-E/SHELL STAR-V-923-AQL

dc.contributor.authorKOKTAY, T
dc.contributor.authorAK, T
dc.contributor.authorKOCER, D
dc.contributor.authorSAYGAC, T
dc.contributor.authorDENIZMAN, L
dc.date.accessioned2021-03-04T11:59:29Z
dc.date.available2021-03-04T11:59:29Z
dc.identifier.citationDENIZMAN L., AK T., KOKTAY T., SAYGAC T., KOCER D., "ON THE FURTHER OBSERVATIONS OF B-E/SHELL STAR-V-923-AQL", ASTROPHYSICS AND SPACE SCIENCE, cilt.222, ss.191-203, 1994
dc.identifier.issn0004-640X
dc.identifier.othervv_1032021
dc.identifier.otherav_75219d2a-0456-40e2-9202-b5c7f498319a
dc.identifier.urihttp://hdl.handle.net/20.500.12627/80472
dc.identifier.urihttps://doi.org/10.1007/bf00627093
dc.description.abstractV 923 Aql is one of the candidate B-e stars to be a binary star. In this research, optical and near-infrared spectral measurements of V 923 Aql is presented. V 923 Aql presents variable H Balmer line profiles with shell components. H alpha profiles present R/V, E/C and radial velocity variation. Shell parameters of the envelope are calculated.
dc.language.isoeng
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleON THE FURTHER OBSERVATIONS OF B-E/SHELL STAR-V-923-AQL
dc.typeMakale
dc.relation.journalASTROPHYSICS AND SPACE SCIENCE
dc.contributor.departmentİstanbul Üniversitesi , ,
dc.identifier.volume222
dc.identifier.startpage191
dc.identifier.endpage203
dc.contributor.firstauthorID20829


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