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dc.contributor.authorMonaco, P
dc.contributor.authorTektunali, FL
dc.contributor.authorMardirossian, F
dc.contributor.authorMezzetti, M
dc.contributor.authorGiuricin, G
dc.date.accessioned2021-03-04T08:20:02Z
dc.date.available2021-03-04T08:20:02Z
dc.identifier.citationGiuricin G., Monaco P., Mardirossian F., Mezzetti M., Tektunali F., "The environmental density and the bulge-to-disk ratio of disk galaxies in the local supercluster", ASTROPHYSICAL LETTERS & COMMUNICATIONS, cilt.33, ss.139-141, 1996
dc.identifier.issn0888-6512
dc.identifier.othervv_1032021
dc.identifier.otherav_62c91da2-fd4d-4f5c-ae88-8cde9fc133f5
dc.identifier.urihttp://hdl.handle.net/20.500.12627/68784
dc.description.abstractRelying on several samples of disk galaxies for which a detailed photometric bulge/disk decomposition has been given in the literature, we have investigated on the relation between the bulge-to-disk light ratio (B/D) and the environmental density. For nearby (z<0.01) galaxies, we provide a well-defined three-dimensional characterization of the local galaxy density. We find that the observed relation between B/D and environmental density simply reflects the average decline of B/D (and bulge luminosity) towards later morphological types coupled with the morphology-density relation. Whenever the latter effect is removed, no primary B/D-density relation is detected. Moreover, unlike previous claims, B/D appears to be unrelated to the galaxy absolute magnitude.
dc.language.isoeng
dc.subjectFizik
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleThe environmental density and the bulge-to-disk ratio of disk galaxies in the local supercluster
dc.typeMakale
dc.relation.journalASTROPHYSICAL LETTERS & COMMUNICATIONS
dc.contributor.department, ,
dc.identifier.volume33
dc.identifier.startpage139
dc.identifier.endpage141
dc.contributor.firstauthorID117166


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