The dependence of oxygen and nitrogen abundances on stellar mass from the CALIFA survey
- E. Pérez-Montero
- R. García-Benito
- J. M. Vílchez
- S. F. Sánchez
- C. Kehrig
- B. Husemann
- S. Duarte Puertas
- J. Iglesias-Páramo
- L. Galbany
- M. Mollá
- C. J. Walcher
- Y. Ascasíbar
- R. M. González Delgado
- R. A. Marino
- J. Masegosa
- E. Pérez
- F. F. Rosales-Ortega
- P. Sánchez-Blázquez
- J. Bland-Hawthorn
- D. Bomans
- Á. R. López-Sánchez
- B. Ziegler
DOIAbstract
Context. The study of the integrated properties of star-forming galaxies is central to understand their formation and evolution. Some of these properties are extensive and therefore their analysis require totally covering and spatially resolved observations. Among these properties, metallicity can be defined in spiral discs by means of integral field spectroscopy (IFS) of individual H i
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