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A 3D analysis of the metal distribution in the compact group of galaxies HCG 31

  • Sergio Torres-Flores
  • , Claudia Mendes De Oliveira
  • , Mayte Alfaro-Cuello
  • , Eleazar Rodrigo Carrasco
  • , Duilia De Mello
  • , Philippe Amram

Research output: Contribution to journalArticlepeer-review

Abstract

We present new Gemini/GMOS integral field unit observations of the central region of the merging compact group of galaxies HCG 31. Using this data set, we derive the oxygen abundances for the merging galaxies HCG 31A and HCG 31C. We found a smooth metallicity gradient between the nuclei of these galaxies, suggesting a mixing of metals between these objects. These results are confirmed by high-resolution Fabry-Perot data, from which we infer that gas is flowing between HCG 31A and HCG 31C.

Original languageEnglish
Pages (from-to)363
Number of pages1
JournalProceedings of the International Astronomical Union
Volume10
DOIs
StatePublished - 2014
Externally publishedYes

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