TY  - JOUR
AU  - Sánchez, S. F.
AU  - Pérez, E.
AU  - Rosales Ortega, F. F.
AU  - Miralles Caballero, D.
AU  - López Sánchez, Á. R.
AU  - Iglesias Páramo, J.
AU  - Marino, Raffaella Anna
AU  - Sánchez Menguiano, L.
AU  - García Benito, R.
AU  - Mast, D.
AU  - Mendoza, M. A.
AU  - Papaderos, P.
AU  - Ellis, S.
AU  - Galbany, L.
AU  - Kehrig, C.
AU  - Monreal Ibero, A.
AU  - González Delgado, R.
AU  - Mollá, M.
AU  - Ziegler, B.
AU  - De Lorenzo Cáceres, A.
AU  - Mendez Abreu, J.
AU  - Bland-Hawthorn, J.
AU  - Bekeraite, S.
AU  - Roth, M. M.
AU  - Pasquali, A.
AU  - Diaz, A.
AU  - Bomans, D.
AU  - van de Ven, G.
AU  - Wisotzki, L.
PY  - 2015
DO  - 10.1051/0004-6361/201424873
SN  - 0004-6361
UR  - https://hdl.handle.net/20.500.14352/23010
T2  - Astronomy & Astrophysics
AB  - Context. H II regions in galaxies are the sites of star formation, so they are special places for understanding the build-up of stellar mass in the universe. The line ratios of this ionized gas are frequently used to characterize the ionization...
LA  - eng
PB  - EDP Sciencies
KW  - Integral field spectroscopy
KW  - Star-forming galaxies
KW  - Mass-metallicity relation
KW  - Spectral energy-distribution
KW  - Potsdam multiaperture spectrophotometer
KW  - Oxygen abundance gradient
KW  - Ionized gaseous nebulae
KW  - Active galactic nuclei
KW  - Small-magellanic-cloud
KW  - Emission-line spectra
TI  - Imprints of galaxy evolution on H II regions: memory of the past uncovered by the CALIFA survey
TY  - journal article
VL  - 574
ER  -