Insights on the Stellar Mass-Metallicity Relation from the CALIFA Survey
- Author(s)
- , R. M. González Delgado, R. Cid Fernandes, R. García-Benito, E. Pérez, A. L. de Amorim, C. Cortijo-Ferrero, E. A. D. Lacerda, R. López Fernández, S. F. Sánchez, N. Vale Asari, J. Alves, J. Bland-Hawthorn, L. Galbany, A. Gallazzi, B. Husemann, S. Bekeraite, B. Jungwiert, A. R. López-Sánchez, A. de Lorenzo-Cáceres, R. A. Marino, D. Mast, M. Mollá, A. del Olmo, P. Sánchez-Blázquez, G. van de Ven, J. M. Vílchez, C. J. Walcher, L. Wisotzki, B. Ziegler
- Abstract
We use spatially and temporally resolved maps of stellar population
properties of 300 galaxies from the CALIFA integral field survey to
investigate how the stellar metallicity (Z sstarf) relates to
the total stellar mass (M sstarf) and the local mass surface
density (μsstarf) in both spheroidal- and disk-dominated
galaxies. The galaxies are shown to follow a clear stellar
mass-metallicity relation (MZR) over the whole
109-1012 M ☉ range. This relation
is steeper than the one derived from nebular abundances, which is
similar to the flatter stellar MZR derived when we consider only young
stars. We also find a strong relation between the local values of
μsstarf and Z sstarf (the μZR), betraying
the influence of local factors in determining Z sstarf. This
shows that both local (μsstarf-driven) and global (M
sstarf-driven) processes are important in determining
metallicity in galaxies. We find that the overall balance between local
and global effects varies with the location within a galaxy. In disks,
μsstarf regulates Z sstarf, producing a strong
μZR whose amplitude is modulated by M sstarf. In spheroids
it is M sstarf that dominates the physics of star formation
and chemical enrichment, with μsstarf playing a minor,
secondary role. These findings agree with our previous analysis of the
star formation histories of CALIFA galaxies, which showed that mean
stellar ages are mainly governed by surface density in galaxy disks and
by total mass in spheroids.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Instituto de Astrofísica de Andalucía (CSIC), Universidade Federal de Santa Catarina, Centro Astronómico Hispano Alemán (CAHA), Universidad Nacional Autonoma de Mexico, The University of Sydney, Universidad de Chile, INAF - Osservatorio Astrofisico di Arcetri, University of Copenhagen, European Southern Observatory (Germany), Leibniz-Institut für Astrophysik Potsdam, Czech Academy of Sciences, Australian Astronomical Observatory, University of St. Andrews, Universidad Complutense de Madrid, Centro Brasileiro de Pesquisas Físicas (CBPF), Centro de Investigaciones Energeticas Medioambientales y Tecnológica, Universidad Autónoma de Madrid, Max-Planck-Institut für Astronomie
- Journal
- The Astrophysical journal Letters
- Volume
- 791
- No. of pages
- 5
- ISSN
- 2041-8205
- DOI
- https://doi.org/10.1088/2041-8205/791/1/L16
- Publication date
- 08-2014
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103003 Astronomy, 103004 Astrophysics
- Keywords
- ASJC Scopus subject areas
- Astronomy and Astrophysics, Space and Planetary Science
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/3acc35b7-e06e-4bde-848f-03a2c8f5566c