Issue |
A&A
Volume 579, July 2015
|
|
---|---|---|
Article Number | A45 | |
Number of page(s) | 9 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/201425397 | |
Published online | 25 June 2015 |
Central star formation and metallicity in CALIFA interacting galaxies
1
Instituto de Astrofísica de Canarias (IAC),
38205, La Laguna, Tenerife, Spain
e-mail:
jkbb@iac.es
2
Depto. Astrofísica, Universidad de La Laguna (ULL),
38206, La Laguna, Tenerife, Spain
3
Instituto de Astronomía,Universidad Nacional Autonóma de
Mexico, A.P.
70-264, 04510,
Mexico
4
Instituto de Cosmologia, Relatividade e Astrofísica – ICRA, Centro Brasileiro de
Pesquisas Físicas, Rua Dr. Xavier Sigaud 150, CEP 22290-180, Rio de Janeiro, RJ, Brazil
5
Instituto de Astrofísica de Andalucía (CSIC),
Glorieta de la Astronomía s/n, Aptdo.
3004, 18080
Granada,
Spain
6
European Southern Observatory (ESO), Karl-Schwarzschild-Str. 2, 85748
Garching b. Muenchen,
Germany
7
Max-Planck-Institut für Astronomie, 69117
Heidelberg,
Germany
8
Estación Experimental de Zonas Aridas (CSIC), Ctra. de Sacramento
s/n, La Cañada, Almería, Spain
9
Instituto Nacional de Astrofísica, Óptica y Electrónica, Luis E. Erro 1,
72840
Tonantzintla, Puebla, Mexico
10
Centro de Estudios de la Física del Cosmos de
Aragón, 44001
Teruel,
Spain
11
CEI Campus Moncloa, UCM-UPM, Departamento de Astrofísica y CC. de
la Atmósfera, Facultad de CC. Físicas, Universidad Complutense de
Madrid, Avda. Complutense
s/n, 28040
Madrid,
Spain
12
Millennium Institute of Astrophysics, Universidad de
Chile, 1058
Santiago,
Chile
13
Departamento de Astronomía, Universidad de Chile,
Casilla 36-D, Santiago, Chile
14
Australian Astronomical Observatory, PO Box 915, North Ryde, NSW
1670,
Australia
15 Department of Physics and Astronomy, Macquarie University,
NSW 2109, Australia
16
Leibniz-Institut für Astrophysik Potsdam (AIP),
An der Sternwarte 16,
14482
Potsdam,
Germany
Received: 24 November 2014
Accepted: 16 April 2015
We use optical integral-field spectroscopic (IFS) data from 103 nearby galaxies at different stages of the merging event, from close pairs to merger remnants provided by the CALIFA survey, to study the impact of the interaction in the specific star formation and oxygen abundance on different galactic scales. To disentangle the effect of the interaction and merger from internal processes, we compared our results with a control sample of 80 non-interacting galaxies. We confirm the moderate enhancement (×2–3 times) of specific star formation for interacting galaxies in central regions as reported by previous studies; however, the specific star formation is comparable when observed in extended regions. We find that control and interacting star-forming galaxies have similar oxygen abundances in their central regions, when normalized to their stellar masses. Oxygen abundances of these interacting galaxies seem to decrease compared to the control objects at the large aperture sizes measured in effective radius. Although the enhancement in central star formation and lower metallicities for interacting galaxies have been attributed to tidally induced inflows, our results suggest that other processes such as stellar feedback can contribute to the metal enrichment in interacting galaxies.
Key words: galaxies: evolution / galaxies: interactions / galaxies: star formation / galaxies: abundances
© ESO, 2015
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