TY  - CHAP
AU  - Aragón Salamanca, A.
AU  - Alonso Herrero, A.
AU  - Gallego Maestro, Jesús
AU  - García Dabó, C. E.
AU  - Pérez González, Pablo Guillermo
AU  - Zamorano Calvo, Jaime
AU  - Gil de Paz, Armando
PY  - 2003
DO  - http://cds.cern.ch/record/584999/files/?ln=es
SN  - 1-58381-144-3
UR  - https://hdl.handle.net/20.500.14352/53497
AB  - The [O ii]λ3727 emission line is frequently used as an indicator of the star formation rate (SFR) despite its complex dependence on metallicity and excitation conditions. We have analysed the properties of the [O II] and Hα emission lines for a...
LA  - eng
M2  - 191
PB  - Astronomical Society of the Pacific
KW  - Madrid survey galaxies
KW  - Nearby field galaxies
KW  - Spectroscopic properties
KW  - Universidad Complutense
KW  - O-II
KW  - Emission
KW  - Photometry
TI  - Star Formation Rate estimators: [O II]λ3727 vs. Hα forlocal star-forming galaxies
TY  - book part
ER  -