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Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images

Kruk, Sandor J.; Lintott, Chris J.; Bamford, Steven P.; Masters, Karen L.; Simmons, Brooke D.; H�u�ler, Boris; Cardamone, Carolin N.; Hart, Ross E.; Schawinski, Kevin; Smethurst, Rebecca J.; Vika, Marina; Kelvin, Lee

Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images Thumbnail


Authors

Sandor J. Kruk

Chris J. Lintott

Karen L. Masters

Brooke D. Simmons

Boris H�u�ler

Carolin N. Cardamone

Ross E. Hart

Kevin Schawinski

Rebecca J. Smethurst

Marina Vika

Lee Kelvin



Abstract

We present the results of two-component (disc+bar) and three-component (disc+bar+bulge) multiwavelength 2D photometric decompositions of barred galaxies in five Sloan Digital Sky Survey (SDSS) bands (ugriz). This sample of ∼3500 nearby (z<0.06) galaxies with strong bars selected from the Galaxy Zoo citizen science project is the largest sample of barred galaxies to be studied using photometric decompositions that include a bar component. With detailed structural analysis, we obtain physical quantities such as the bar- and bulge-to-total luminosity ratios, effective radii, Sersic indices and colours of the individual components. We observe a clear difference in the colours of the components, the discs being bluer than the bars and bulges. An overwhelming fraction of bulge components have Sersic indices consistent with being pseudo-bulges. By comparing the barred galaxies with a mass-matched and volume-limited sample of unbarred galaxies, we examine the connection between the presence of a large-scale galactic bar and the properties of discs and bulges. We find that the discs of unbarred galaxies are significantly bluer compared to the discs of barred galaxies, while there is no significant difference in the colours of the bulges. We find possible evidence of secular evolution via bars that leads to the build-up of pseudo-bulges and to the quenching of star formation in the discs. We identify a subsample of unbarred galaxies with an inner lens/oval and find that their properties are similar to barred galaxies, consistent with an evolutionary scenario in which bars dissolve into lenses. This scenario deserves further investigation through both theoretical and observational work.

Citation

Kruk, S. J., Lintott, C. J., Bamford, S. P., Masters, K. L., Simmons, B. D., Häußler, B., Cardamone, C. N., Hart, R. E., Schawinski, K., Smethurst, R. J., Vika, M., & Kelvin, L. (2018). Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images. Monthly Notices of the Royal Astronomical Society, 473(4), https://doi.org/10.1093/mnras/stx2605

Journal Article Type Article
Acceptance Date Oct 4, 2017
Online Publication Date Oct 9, 2017
Publication Date Mar 1, 2018
Deposit Date Jan 4, 2018
Publicly Available Date Jan 4, 2018
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 473
Issue 4
DOI https://doi.org/10.1093/mnras/stx2605
Keywords galaxies: bulges ; galaxies: evolution ; galaxies: general ; galaxies: star formation ; galaxies: stellar content ; galaxies: structure
Public URL https://nottingham-repository.worktribe.com/output/918285
Publisher URL https://academic.oup.com/mnras/article/473/4/4731/4411828
Contract Date Jan 4, 2018

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