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dc.contributor.authorTEKTUNALI, FL
dc.contributor.authorTEKTUNALI, HG
dc.date.accessioned2021-03-03T18:55:38Z
dc.date.available2021-03-03T18:55:38Z
dc.date.issued1991
dc.identifier.citationTEKTUNALI F., TEKTUNALI H., "DEPENDENCE OF CERTAIN ROTATIONAL PROPERTIES OF 78 SPIRAL GALAXIES ON HUBBLE TYPE AND LUMINOSITY", ASTROPHYSICS AND SPACE SCIENCE, cilt.183, sa.1, ss.155-162, 1991
dc.identifier.issn0004-640X
dc.identifier.otherav_51c3a56c-7ed5-4af8-9b7a-895f557757cd
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/58108
dc.identifier.urihttps://doi.org/10.1007/bf00643024
dc.description.abstractDependence of the central velocity gradients on Hubble's type is presented for 78 spiral galaxies with existing rotation curves. Also the dependence of the maximum rotational velocities of 27 galaxies on both Hubble's type and the luminosity is studied. The central velocity gradient is shown to be related with Hubble's type. Maximum rotational velocities of 27 galaxies of our sample depend on Hubble's type such that the mean values of maximum rotational velocity decrease from Sa through Sc. It is also determined that there is a dependence of the maximum rotational velocity on the absolute blue magnitude for each intrinsic Hubble type. For each Hubble type, maximum rotational velocity increases with increasing absolute blue magnitudes.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleDEPENDENCE OF CERTAIN ROTATIONAL PROPERTIES OF 78 SPIRAL GALAXIES ON HUBBLE TYPE AND LUMINOSITY
dc.typeMakale
dc.relation.journalASTROPHYSICS AND SPACE SCIENCE
dc.contributor.department, ,
dc.identifier.volume183
dc.identifier.issue1
dc.identifier.startpage155
dc.identifier.endpage162
dc.contributor.firstauthorID113021


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