Studying the Interstellar Medium of H II-BCD Galaxies Using IFU SpectroscopyReport as inadecuate




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Advances in AstronomyVolume 2013 2013, Article ID 631943, 9 pages

Research ArticleCentro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal

Received 19 April 2013; Accepted 23 July 2013

Academic Editor: Jorge Iglesias Páramo

Copyright © 2013 Patricio Lagos and Polychronis Papaderos. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Abstract

We review the results from our studies, and previous published work, on the spatially resolved physical properties of a sample of H II-BCD galaxies, as obtained mainly from integral-field unit spectroscopy with Gemini-GMOS and VLT-VIMOS. We confirm that, within observational uncertainties, our sample galaxies show nearly spatially constant chemical abundances similar to other low-mass starburst galaxies. They also show He II   4686 emission with the properties being suggestive of a mix of excitation sources and with Wolf-Rayet stars being excluded as the primary ones. Finally, in this contribution, we include a list of all H II-BCD galaxies studied thus far with integral-field unit spectroscopy.





Author: Patricio Lagos and Polychronis Papaderos

Source: https://www.hindawi.com/



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