Exploring the impact of galactic interactions and mergers on the central oxygen abundance of APEX/EDGE–CALIFA galaxies

Author:

Garay-Solis Y1ORCID,Barrera-Ballesteros J K1ORCID,Carigi L1ORCID,Colombo D2,Sánchez S F3ORCID,Lugo-Aranda A Z1,Villanueva V4,Wong T5,Bolatto A D6

Affiliation:

1. Instituto de Astronomía, Universidad Nacional Autónoma de México , A.P. 70-264, 04510 CDMX , México

2. Argelander-Institut für Astronomie , University of Bonn, Auf dem Hügel 71, D-53121 Bonn , Germany

3. Instituto de Astronomía, Universidad Nacional Autónoma de México , A.P. 106, Ensenada, 22800 BC , México

4. Departamento de Astronomía, Universidad de Concepción, Barrio Universitario , Concepción , Chile

5. Department of Astronomy, University of Illinois , Urbana, IL 61801 , USA

6. Department of Astronomy, University of Maryland , College Park, MD 20742 , USA

Abstract

ABSTRACT In this study, we explore the impact of the galactic interaction/mergers on the central oxygen abundance. We analyse 234 star-forming galaxies included in the Calar Alto Legacy Integral Field Area survey with integrated molecular gas observations from the Atacama Pathfinder EXperiment millimeter telescope and the CARMA interferometer. This database has the most optical integral field spectroscopy data with CO data for yet, with integrated measurements within $\sim 1~{R_{\rm{eff}}}$. Our sample includes 125 isolated galaxies (control sample) and 109 galaxies in different merging stages. We find that despite whether the merging galaxies show an increase or decrease in their molecular gas fraction, the oxygen abundance does not vary significantly, in comparison to our control sample. Therefore, the enhancement and suppression of oxygen abundance are similar in both isolated galaxies and interacting/merging galaxies. On the contrary, regardless of the merger stage (including isolated sample), galaxies that present an increase in their specific star formation rate present a metallicity dilution. We suggest that both internal and external events affect the chemical composition of merging galaxies.

Funder

NSF

CONACYT

Publisher

Oxford University Press (OUP)

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