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THE LOCAL GALAXY DENSITY AND THE BULGE-TO-DISK RATIO OF DISK GALAXIES

dc.contributor.authorTEKTUNALI, FL
dc.contributor.authorMEZZETTI, M
dc.contributor.authorMONACO, P
dc.contributor.authorMARDIROSSIAN, F
dc.contributor.authorGIURICIN, G
dc.date.accessioned2021-03-05T11:44:45Z
dc.date.available2021-03-05T11:44:45Z
dc.date.issued1995
dc.identifier.citationGIURICIN G., TEKTUNALI F., MONACO P., MARDIROSSIAN F., MEZZETTI M., "THE LOCAL GALAXY DENSITY AND THE BULGE-TO-DISK RATIO OF DISK GALAXIES", ASTROPHYSICAL JOURNAL, cilt.450, ss.41-50, 1995
dc.identifier.issn0004-637X
dc.identifier.othervv_1032021
dc.identifier.otherav_a9b5d7e0-4d87-40c9-8d12-ba4769fe16ff
dc.identifier.urihttp://hdl.handle.net/20.500.12627/113352
dc.identifier.urihttps://doi.org/10.1086/176117
dc.description.abstractRelying on samples of disk galaxies for which a detailed photometric bulge/disk decomposition has been provided in the literature, we examine the dependence of the bulge-to-disk luminosity ratio (B/D) on the blue absolute luminosity and on the environmental density. In our statistical analysis of various B/D data sets we pay particular attention to disentangling the role played by the galaxy morphology-galaxy density relation. Besides, we focus our attention on nearby (z < 0.01) galaxies, for which we can provide a three-dimensional characterization of the local galaxy density.
dc.language.isoeng
dc.subjectUzay bilimi
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.titleTHE LOCAL GALAXY DENSITY AND THE BULGE-TO-DISK RATIO OF DISK GALAXIES
dc.typeMakale
dc.relation.journalASTROPHYSICAL JOURNAL
dc.contributor.department, ,
dc.identifier.volume450
dc.identifier.issue1
dc.identifier.startpage41
dc.identifier.endpage50
dc.contributor.firstauthorID116610


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