Interaction effects on galaxy pairs with Gemini/GMOS - II: oxygen abundance gradients

In this paper we derived oxygen abundance gradients from HII regions located in eleven galaxies in eight systems of close pairs. Long-slit spectra in the range 4400-7300 Å were obtained with the Gemini Multi-Object Spectrograph at Gemini South (GMOS). Spatial profiles of oxygen abundance in the gase...

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Autores principales: Rosa, D. A., Dors, Oli L., Krabbe, A. C., Hägele, Guillermo Federico, Cardaci, Mónica Viviana, Pastoriza, Miriani Griselda, Rodrigues, Irapuan, Winge, Claudia
Formato: Articulo
Lenguaje:Inglés
Publicado: 2014
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/127166
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id I19-R120-10915-127166
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
techniques: imaging spectroscopy
ISM: abundances
galaxies: abundances
galaxies: interactions
spellingShingle Astronomía
techniques: imaging spectroscopy
ISM: abundances
galaxies: abundances
galaxies: interactions
Rosa, D. A.
Dors, Oli L.
Krabbe, A. C.
Hägele, Guillermo Federico
Cardaci, Mónica Viviana
Pastoriza, Miriani Griselda
Rodrigues, Irapuan
Winge, Claudia
Interaction effects on galaxy pairs with Gemini/GMOS - II: oxygen abundance gradients
topic_facet Astronomía
techniques: imaging spectroscopy
ISM: abundances
galaxies: abundances
galaxies: interactions
description In this paper we derived oxygen abundance gradients from HII regions located in eleven galaxies in eight systems of close pairs. Long-slit spectra in the range 4400-7300 Å were obtained with the Gemini Multi-Object Spectrograph at Gemini South (GMOS). Spatial profiles of oxygen abundance in the gaseous phase along galaxy disks were obtained using calibrations based on strong emission-lines (N2 and O3N2). We found oxygen gradients significantly flatter for all the studied galaxies than those in typical isolated spiral galaxies. Four objects in our sample, AM1219A, AM1256B, AM 2030A and AM2030B, show a clear break in the oxygen abundance at galactocentric radius R/R₂₅ between 0.2 and 0.5. For AM1219A and AM1256B we found negative slopes for the inner gradients, and for AM2030B we found a positive one. In all these three cases they show a flatter behaviour to the outskirts of the galaxies. For AM2030A, we found a positive-slope outer gradient while the inner one is almost compatible with a flat behaviour. A decrease of star formation efficiency in the zone that corresponds to the oxygen abundance gradient break for AM1219A and AM2030B was found. For the former, a minimum in the estimated metallicities was found very close to the break zone that could be associated with a corotation radius. On the other hand, AM1256B and AM2030A, present a SFR maximum but not an extreme oxygen abundance value. All the four interacting systems that show oxygen gradient breakes the extreme SFR values are located very close to break zones. Hii regions located in close pairs of galaxies follow the same relation between the ionization parameter and the oxygen abundance as those regions in isolated galaxies.
format Articulo
Articulo
author Rosa, D. A.
Dors, Oli L.
Krabbe, A. C.
Hägele, Guillermo Federico
Cardaci, Mónica Viviana
Pastoriza, Miriani Griselda
Rodrigues, Irapuan
Winge, Claudia
author_facet Rosa, D. A.
Dors, Oli L.
Krabbe, A. C.
Hägele, Guillermo Federico
Cardaci, Mónica Viviana
Pastoriza, Miriani Griselda
Rodrigues, Irapuan
Winge, Claudia
author_sort Rosa, D. A.
title Interaction effects on galaxy pairs with Gemini/GMOS - II: oxygen abundance gradients
title_short Interaction effects on galaxy pairs with Gemini/GMOS - II: oxygen abundance gradients
title_full Interaction effects on galaxy pairs with Gemini/GMOS - II: oxygen abundance gradients
title_fullStr Interaction effects on galaxy pairs with Gemini/GMOS - II: oxygen abundance gradients
title_full_unstemmed Interaction effects on galaxy pairs with Gemini/GMOS - II: oxygen abundance gradients
title_sort interaction effects on galaxy pairs with gemini/gmos - ii: oxygen abundance gradients
publishDate 2014
url http://sedici.unlp.edu.ar/handle/10915/127166
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