Keunho Kim
The demographics of galactic bulges in the SDSS database
Kim, Keunho; Oh, Sree; Jeong, Hyunjin; Arag�n-Salamanca, Alfonso; Smith, Rory; Yi, Sukyoung K.
Authors
Sree Oh
Hyunjin Jeong
Professor ALFONSO ARAGON-SALAMANCA ALFONSO.ARAGON@NOTTINGHAM.AC.UK
PROFESSOR OF ASTRONOMY
Rory Smith
Sukyoung K. Yi
Abstract
We present a new database of our two-dimensional bulge–disk decompositions for 14,233 galaxies drawn from Sloan Digital Sky Survey DR12 in order to examine the properties of bulges residing in the local universe (0.005 < z < 0.05). We performed decompositions in the g and r bands by utilizing the galfit software. The bulge colors and bulge-to-total ratios are found to be sensitive to the details in the decomposition technique, and hence we hereby provide full details of our method. The g − r colors of bulges derived are almost constantly red regardless of bulge size, except for the bulges in the low bulge-to-total ratio galaxies (B/T r lesssim 0.3). Bulges exhibit similar scaling relations to those followed by elliptical galaxies, but the bulges in galaxies with lower bulge-to-total ratios clearly show a gradually larger departure in slope from the elliptical galaxy sequence. The scatters around the scaling relations are also larger for the bulges in galaxies with lower bulge-to-total ratios. Both the departure in slopes and larger scatters likely originate from the presence of young stars. The bulges in galaxies with low bulge-to-total ratios show signs of a frosting of young stars so substantial that their luminosity-weighted Balmer-line ages are as small as 1 Gyr in some cases. While bulges seem largely similar in optical properties to elliptical galaxies, they do show clear and systematic departures as a function of bulge-to-total ratio. The stellar properties and perhaps associated formation processes of bulges seem much more diverse than those of elliptical galaxies.
Citation
Kim, K., Oh, S., Jeong, H., Aragón-Salamanca, A., Smith, R., & Yi, S. K. (2016). The demographics of galactic bulges in the SDSS database. Astrophysical Journal Supplement, 225(1), Article 6. https://doi.org/10.3847/0067-0049/225/1/6
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 21, 2016 |
Publication Date | Jul 13, 2016 |
Deposit Date | Jan 10, 2017 |
Publicly Available Date | Jan 10, 2017 |
Journal | Astrophysical Journal Supplement Series |
Print ISSN | 0067-0049 |
Electronic ISSN | 1538-4365 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 225 |
Issue | 1 |
Article Number | 6 |
DOI | https://doi.org/10.3847/0067-0049/225/1/6 |
Keywords | galaxies: bulges; galaxies: elliptical and lenticular, cD; galaxies: formation; galaxies: spiral; galaxies: stellar content; galaxies: structure |
Public URL | https://nottingham-repository.worktribe.com/output/801154 |
Publisher URL | http://iopscience.iop.org/article/10.3847/0067-0049/225/1/6/meta; |
Contract Date | Jan 10, 2017 |
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Kim_2016_ApJS_225_6(1).pdf
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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf
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