Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images
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 Z...
| Main Authors: | , , , , , , , , , , , |
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| Format: | Article |
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Oxford University Press
2018
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| Online Access: | https://eprints.nottingham.ac.uk/48932/ |
| _version_ | 1848797882340081664 |
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| author | Kruk, Sandor J. Lintott, Chris J. Bamford, Steven P. Masters, Karen L. Simmons, Brooke D. Häußler, Boris Cardamone, Carolin N. Hart, Ross E. Kelvin, Lee Schawinski, Kevin Smethurst, Rebecca J. Vika, Marina |
| author_facet | Kruk, Sandor J. Lintott, Chris J. Bamford, Steven P. Masters, Karen L. Simmons, Brooke D. Häußler, Boris Cardamone, Carolin N. Hart, Ross E. Kelvin, Lee Schawinski, Kevin Smethurst, Rebecca J. Vika, Marina |
| author_sort | Kruk, Sandor J. |
| building | Nottingham Research Data Repository |
| collection | Online Access |
| description | 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. |
| first_indexed | 2025-11-14T20:10:56Z |
| format | Article |
| id | nottingham-48932 |
| institution | University of Nottingham Malaysia Campus |
| institution_category | Local University |
| last_indexed | 2025-11-14T20:10:56Z |
| publishDate | 2018 |
| publisher | Oxford University Press |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | nottingham-489322024-08-15T15:27:09Z https://eprints.nottingham.ac.uk/48932/ 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. Häußler, Boris Cardamone, Carolin N. Hart, Ross E. Kelvin, Lee Schawinski, Kevin Smethurst, Rebecca J. Vika, Marina 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. Oxford University Press 2018-03-01 Article PeerReviewed Kruk, Sandor J., Lintott, Chris J., Bamford, Steven P., Masters, Karen L., Simmons, Brooke D., Häußler, Boris, Cardamone, Carolin N., Hart, Ross E., Kelvin, Lee, Schawinski, Kevin, Smethurst, Rebecca J. and Vika, Marina (2018) Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images. Monthly Notices of the Royal Astronomical Society, 473 (4). pp. 4731-4753. ISSN 1365-2966 galaxies: bulges ; galaxies: evolution ; galaxies: general ; galaxies: star formation ; galaxies: stellar content ; galaxies: structure https://academic.oup.com/mnras/article/473/4/4731/4411828 doi:10.1093/mnras/stx2605 doi:10.1093/mnras/stx2605 |
| spellingShingle | galaxies: bulges ; galaxies: evolution ; galaxies: general ; galaxies: star formation ; galaxies: stellar content ; galaxies: structure Kruk, Sandor J. Lintott, Chris J. Bamford, Steven P. Masters, Karen L. Simmons, Brooke D. Häußler, Boris Cardamone, Carolin N. Hart, Ross E. Kelvin, Lee Schawinski, Kevin Smethurst, Rebecca J. Vika, Marina Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images |
| title | Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images |
| title_full | Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images |
| title_fullStr | Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images |
| title_full_unstemmed | Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images |
| title_short | Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images |
| title_sort | galaxy zoo: secular evolution of barred galaxies from structural decomposition of multiband images |
| topic | galaxies: bulges ; galaxies: evolution ; galaxies: general ; galaxies: star formation ; galaxies: stellar content ; galaxies: structure |
| url | https://eprints.nottingham.ac.uk/48932/ https://eprints.nottingham.ac.uk/48932/ https://eprints.nottingham.ac.uk/48932/ |