Galaxy Zoo: finding offset discs and bars in SDSS galaxies

We use multiwavelength Sloan Digital Sky Survey (SDSS) images and Galaxy Zoo morphologies to identify a sample of ∼270 late-type galaxies with an off-centre bar. We measure offsets in the range 0.2–2.5 kpc between the photometric centres of the stellar disc and stellar bar. The measured offsets corr...

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Main Authors: Kruk, Sandor J., Lintott, Chris J., Simmons, Brooke D., Bamford, Steven P., Cardamone, Carolin N., Fortson, Lucy, Hart, Ross E., Häußler, Boris, Masters, Karen L., Nichol, Robert C., Schawinski, Kevin, Smethurst, Rebecca J.
Format: Article
Published: Oxford University Press 2017
Subjects:
Online Access:https://eprints.nottingham.ac.uk/43548/
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author Kruk, Sandor J.
Lintott, Chris J.
Simmons, Brooke D.
Bamford, Steven P.
Cardamone, Carolin N.
Fortson, Lucy
Hart, Ross E.
Häußler, Boris
Masters, Karen L.
Nichol, Robert C.
Schawinski, Kevin
Smethurst, Rebecca J.
author_facet Kruk, Sandor J.
Lintott, Chris J.
Simmons, Brooke D.
Bamford, Steven P.
Cardamone, Carolin N.
Fortson, Lucy
Hart, Ross E.
Häußler, Boris
Masters, Karen L.
Nichol, Robert C.
Schawinski, Kevin
Smethurst, Rebecca J.
author_sort Kruk, Sandor J.
building Nottingham Research Data Repository
collection Online Access
description We use multiwavelength Sloan Digital Sky Survey (SDSS) images and Galaxy Zoo morphologies to identify a sample of ∼270 late-type galaxies with an off-centre bar. We measure offsets in the range 0.2–2.5 kpc between the photometric centres of the stellar disc and stellar bar. The measured offsets correlate with global asymmetries of the galaxies, with those with largest offsets showing higher lopsidedness. These findings are in good agreement with predictions from simulations of dwarf–dwarf tidal interactions producing off-centre bars. We find that the majority of galaxies with off-centre bars are of Magellanic type, with a median mass of 109.6 M⊙, and 91 per cent of them having M⋆ < 3 × 1010 M⊙, the characteristic mass at which galaxies start having higher central concentrations attributed to the presence of bulges. We conduct a search for companions to test the hypothesis of tidal interactions, but find that a similar fraction of galaxies with offset bars have companions within 100 kpc as galaxies with centred bars. Although this may be due to the incompleteness of the SDSS spectroscopic survey at the faint end, alternative scenarios that give rise to offset bars such as interactions with dark companions or the effect of lopsided halo potentials should be considered. Future observations are needed to confirm possible low-mass companion candidates and to determine the shape of the dark matter halo, in order to find the explanation for the off-centre bars in these galaxies.
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spelling nottingham-435482020-05-04T19:56:17Z https://eprints.nottingham.ac.uk/43548/ Galaxy Zoo: finding offset discs and bars in SDSS galaxies Kruk, Sandor J. Lintott, Chris J. Simmons, Brooke D. Bamford, Steven P. Cardamone, Carolin N. Fortson, Lucy Hart, Ross E. Häußler, Boris Masters, Karen L. Nichol, Robert C. Schawinski, Kevin Smethurst, Rebecca J. We use multiwavelength Sloan Digital Sky Survey (SDSS) images and Galaxy Zoo morphologies to identify a sample of ∼270 late-type galaxies with an off-centre bar. We measure offsets in the range 0.2–2.5 kpc between the photometric centres of the stellar disc and stellar bar. The measured offsets correlate with global asymmetries of the galaxies, with those with largest offsets showing higher lopsidedness. These findings are in good agreement with predictions from simulations of dwarf–dwarf tidal interactions producing off-centre bars. We find that the majority of galaxies with off-centre bars are of Magellanic type, with a median mass of 109.6 M⊙, and 91 per cent of them having M⋆ < 3 × 1010 M⊙, the characteristic mass at which galaxies start having higher central concentrations attributed to the presence of bulges. We conduct a search for companions to test the hypothesis of tidal interactions, but find that a similar fraction of galaxies with offset bars have companions within 100 kpc as galaxies with centred bars. Although this may be due to the incompleteness of the SDSS spectroscopic survey at the faint end, alternative scenarios that give rise to offset bars such as interactions with dark companions or the effect of lopsided halo potentials should be considered. Future observations are needed to confirm possible low-mass companion candidates and to determine the shape of the dark matter halo, in order to find the explanation for the off-centre bars in these galaxies. Oxford University Press 2017-08 Article PeerReviewed Kruk, Sandor J., Lintott, Chris J., Simmons, Brooke D., Bamford, Steven P., Cardamone, Carolin N., Fortson, Lucy, Hart, Ross E., Häußler, Boris, Masters, Karen L., Nichol, Robert C., Schawinski, Kevin and Smethurst, Rebecca J. (2017) Galaxy Zoo: finding offset discs and bars in SDSS galaxies. Monthly Notices of the Royal Astronomical Society, 469 (3). pp. 3363-3373. ISSN 1365-2966 galaxies: dwarf galaxies: evolution galaxies: interactions galaxies: irregular galaxies: structure https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stx1026 doi:10.1093/mnras/stx1026 doi:10.1093/mnras/stx1026
spellingShingle galaxies: dwarf
galaxies: evolution
galaxies: interactions
galaxies: irregular
galaxies: structure
Kruk, Sandor J.
Lintott, Chris J.
Simmons, Brooke D.
Bamford, Steven P.
Cardamone, Carolin N.
Fortson, Lucy
Hart, Ross E.
Häußler, Boris
Masters, Karen L.
Nichol, Robert C.
Schawinski, Kevin
Smethurst, Rebecca J.
Galaxy Zoo: finding offset discs and bars in SDSS galaxies
title Galaxy Zoo: finding offset discs and bars in SDSS galaxies
title_full Galaxy Zoo: finding offset discs and bars in SDSS galaxies
title_fullStr Galaxy Zoo: finding offset discs and bars in SDSS galaxies
title_full_unstemmed Galaxy Zoo: finding offset discs and bars in SDSS galaxies
title_short Galaxy Zoo: finding offset discs and bars in SDSS galaxies
title_sort galaxy zoo: finding offset discs and bars in sdss galaxies
topic galaxies: dwarf
galaxies: evolution
galaxies: interactions
galaxies: irregular
galaxies: structure
url https://eprints.nottingham.ac.uk/43548/
https://eprints.nottingham.ac.uk/43548/
https://eprints.nottingham.ac.uk/43548/