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Outer-disk reddening and gas-phase metallicities: The CALIFA connection

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  • معلومة اضافية
    • بيانات النشر:
      EDP Sciencies
    • الموضوع:
      2016
    • Collection:
      Universidad Complutense de Madrid (UCM): E-Prints Complutense
    • الموضوع:
      52
    • نبذة مختصرة :
      We study, for the first time in a statistically significant and well-defined sample, the relation between the outer-disk ionized-gas metallicity gradients and the presence of breaks in the surface brightness profiles of disk galaxies. Sloan Digital Sky Survey (SDSS) g′- and r′-band surface brightness, (g′ – r′) color, and ionized-gasoxygen abundance profiles for 324 galaxies within the Calar Alto Legacy Integral Field Area (CALIFA) survey are used for this purpose. We perform a detailed light-profile classification, finding that 84% of our disks show down- or up-bending profiles (Type II and Type III, respectively), while the remaining 16% are well fitted by one single exponential (Type I). The analysis of the color gradients at both sides of this break shows a U-shaped profile for most Type II galaxies with an average minimum (g′ − r′) color of ~0.5 mag and an ionized-gas metallicity flattening associated with it only in the case of low-mass galaxies. Comparatively, more massive systems show a rather uniform negative metallicity gradient. The correlation between metallicity flattening and stellar mass for these systems results in p-values as low as 0.01. Independent of the mechanism having shaped the outer light profiles of these galaxies, stellar migration or a previous episode of star formation in a shrinking star-forming disk, it is clear that the imprint in their ionized-gas metallicity was different for low- and high-mass Type II galaxies. In the case of Type III disks, a positive correlation between the change in color and abundance gradient is found (the null hypothesis is ruled out with a p-value of 0.02), with the outer disks of Type III galaxies with masses ≤10^10 M_⊙ showing a weak color reddening or even a bluing. This is interpreted as primarily due to a mass downsizing effect on the population of Type III galaxies that recently experienced an enhanced inside-out growth. ; Unión Europea - FP7 ; Ministerio de Economía, Comercio y Empresa (España) ; Campus de Excelencia Internacional Moncloa ; Unión ...
    • File Description:
      application/pdf
    • ISSN:
      1432-0746
    • Relation:
      SFEHG (303912); DAGAL (289313); AyA2010-15081; AyA2012-30717; AyA2013-46724P; IC 120009; 3140566; IF/01220/2013; FCOMP-01-0124-FEDER-029170; FCT PTDC/FIS-AST/3214/2012; CONACYT-125180; DGAPA-IA100815; Marino, R. A., Gil de Paz, A., Sánchez, S. F. et al. «Outer-Disk Reddening and Gas-Phase Metallicities: The CALIFA Connection». Astronomy & Astrophysics, vol. 585, enero de 2016, p. A47. www.aanda.org, https://doi.org/10.1051/0004-6361/201526986.; https://hdl.handle.net/20.500.14352/24440
    • الرقم المعرف:
      10.1051/0004-6361/201526986
    • الدخول الالكتروني :
      https://hdl.handle.net/20.500.14352/24440
      https://doi.org/10.1051/0004-6361/201526986
    • Rights:
      open access
    • الرقم المعرف:
      edsbas.1531294C