Skip to main content

The effect of environment on discs and bulges

Author(s): Lackner, CN; Gunn, James E

Download
To refer to this page use: http://arks.princeton.edu/ark:/88435/pr1x05xc11
Full metadata record
DC FieldValueLanguage
dc.contributor.authorLackner, CN-
dc.contributor.authorGunn, James E-
dc.date.accessioned2022-01-25T14:58:33Z-
dc.date.available2022-01-25T14:58:33Z-
dc.date.issued2013-01en_US
dc.identifier.citationLackner, CN, Gunn, JE. (2013). The effect of environment on discs and bulges. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 428 (2141 - 2162. doi:10.1093/mnras/sts179en_US
dc.identifier.issn0035-8711-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1x05xc11-
dc.description.abstractWe examine the changes in the properties of galactic bulges and discs with environment for a volume-limited sample of 12 500 nearby galaxies from Sloan Digital Sky Survey. We focus on galaxies with classical bulges. Classical bulges seem to have the same formation history as ellipticals of the same mass, and we test if environment determines whether or not a classical bulge possesses a disc. Using the projected fifth nearest neighbour density as a measure of local environment, we look for correlations with environment at fixed bulge stellar mass. In groups with fewer than 20 members, we find no evidence for changes in disc morphology with local density. At fixed bulge mass, disc mass and disc scalelength are independent of local density. However, disc colour does increase [Delta(g - r) similar to 0.05 mag] as a function of local density in relatively poor groups. Therefore, the colour-density relation for classical bulge+disc galaxies in the field and in poor groups is solely due to changes in disc colour with density. In contrast, we find no correlations between disc colour and local density for classical bulge+disc galaxies in large, relaxed groups and clusters. However, there is a weak correlation between disc mass and group crossing time, suggesting that morphological transformation takes places in rich groups. Our results add to the evidence that star formation is quenched in group environments, instead of clusters, and that star formation quenching and morphological transformation are separate processes. Overall, we show that environment has two effects on galactic discs: relatively low-density environments can quench star formation in discs, while processes occurring in higher density environments contribute to the morphological transformation from disc-dominated systems to bulge-dominated systems.en_US
dc.format.extent2141 - 2162en_US
dc.language.isoen_USen_US
dc.relationhttps://ui.adsabs.harvard.edu/abs/2013MNRAS.428.2141L/abstracten_US
dc.relation.ispartofMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleThe effect of environment on discs and bulgesen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1093/mnras/sts179-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

Files in This Item:
File Description SizeFormat 
sts179.pdf1.95 MBAdobe PDFView/Download


Items in OAR@Princeton are protected by copyright, with all rights reserved, unless otherwise indicated.