Hostname: page-component-7479d7b7d-qlrfm Total loading time: 0 Render date: 2024-07-11T01:18:27.397Z Has data issue: false hasContentIssue false
  • English
  • Français

Gas and stellar metallicity gradients in face-on disc galaxies

Published online by Cambridge University Press:  03 March 2020

P. Sánchez-Blázquez
P. Sánchez-Blázquez*
Affiliation:
Universidad Autónoma de Madrid, 28049, Madrid, Spain
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present an analysis of the stellar and gaseous metallicity gradients in a sample of 260 disc galaxies from the CALIFA survey. The slope of the different components are compared with the main characteristics of the galaxies, such as mass, morphology, presence of a bar, or gas fraction.

Keywords

galaxies: stellar contentgalaxies: evolutiongalaxies: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 261 - 262
Copyright
© International Astronomical Union 2020

References

Lian, J., Thomas, D., Maraston, C., et al. 2018, MNRAS, 476, 3883 CrossRefGoogle Scholar
Sánchez, S. F., Kennicutt, R., Gil de Paz, A., et al. 2012, A&A, 538, 8 Google Scholar