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Ciencias Astronómicas
6
Galaxies: starburst
4
H ii regions
3
ISM: abundances
3
Galaxies: kinematics and dynamics
2
Galaxies: star clusters
2
Galaxies: stellar content
2
H II regions
2
galaxies: abundances
2
Física
1
Galaxies: abundances
1
Galaxies: fundamental parameters
1
Galaxies: individual: NGC 2903
1
Galaxies: individual: NGC 3310
1
galaxies: ISM
1
galaxies: evolution
1
galaxies: formation
1
galaxies: general
1
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1por Zinchenko, Igor A., Dors, Oli L., Hägele, Guillermo Federico, Cardaci, Mónica Viviana, Krabbe, Angela“... of these parameters in each galactic disc for the objects in our sample. Most of the galaxies in our sample (∼70 per...”
Publicado 2018
Aportado por: SEDICI (UNLP)Articulo -
2por Hägele, Guillermo Federico, Díaz Beltrán, Ángeles Isabel, Cardaci, Mónica Viviana, Terlevich, Elena, Terlevich, Roberto“... per cent of the total dynamical mass.The ionized gas kinematics is complex; two different kinematical...”
Publicado 2010
Aportado por: SEDICI (UNLP)Articulo -
3“... per cent) present Teff values in the range between 37 and 40 kK, with an average value of 38.5(±1) kK...”
Aportado por: SEDICI (UNLP)Articulo Preprint -
4Disentangling the metallicity and star formation history of H ii galaxies through tailor-made modelspor Pérez Montero, Enrique, García Benito, Rubén, Hägele, Guillermo Federico, Díaz Beltrán, Ángeles Isabel“... of the underlying stellar population to the equivalent width of Hβ [EW(Hβ)], which amounts to about 10 per cent...”
Publicado 2010
Aportado por: SEDICI (UNLP)Articulo -
5Abundance determination of multiple star-forming regions in the H II galaxy SDSS J165712.75+321141.4por Hägele, Guillermo Federico, García Benito, Rubén, Pérez Montero, Enrique, Díaz, Ángeles I., Cardaci, Mónica Viviana, Firpo, Verónica, Terlevich, Elena, Terlevich, Roberto“...]) and Te([S II]) - with high-precision, rms errors of the order of 2, 5, 6 and 6 per cent, respectively...”
Publicado 2011
Aportado por: SEDICI (UNLP)Articulo -
6por Hägele, Guillermo Federico, Díaz Beltrán, Ángeles Isabel, Cardaci, Mónica Viviana, Terlevich, Elena, Terlevich, Roberto“... nucleus, therefore constituting between 1 and 4 per cent of the total dynamical mass. In the CNSFR, star...”
Publicado 2009
Aportado por: SEDICI (UNLP)Articulo