The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era

A new generation of wide-field emission-line surveys based on integral field units (IFU) is allowing us to obtain spatially resolved information of the gas-phase emission in nearby late-type galaxies, based on large samples of HII regions and full two-dimensional coverage. These observations are all...

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Main Author: Fernando Fabián Rosales-Ortega
Format: Article
Language:English
Published: Wiley 2013-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2013/627867
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author Fernando Fabián Rosales-Ortega
author_facet Fernando Fabián Rosales-Ortega
author_sort Fernando Fabián Rosales-Ortega
collection DOAJ
description A new generation of wide-field emission-line surveys based on integral field units (IFU) is allowing us to obtain spatially resolved information of the gas-phase emission in nearby late-type galaxies, based on large samples of HII regions and full two-dimensional coverage. These observations are allowing us to discover and characterise abundance differentials between galactic substructures and new scaling relations with global physical properties. Here I review some highlights of our current studies employing this technique: (1) the case study of NGC 628, the largest galaxy ever sampled with an IFU; (2) a statistical approach to the abundance gradients of spiral galaxies, which indicates a universal radial gradient for oxygen abundance; and (3) the discovery of a new scaling relation of HII regions in spiral galaxies, the local mass-metallicity relation of star-forming galaxies. The observational properties and constrains found in local galaxies using this new technique will allow us to interpret the gas-phase abundance of analogue high-z systems.
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spelling doaj-art-c4796d9dc4794f2e96c2fa60dbbab8ab2025-02-03T06:10:49ZengWileyAdvances in Astronomy1687-79691687-79772013-01-01201310.1155/2013/627867627867The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU EraFernando Fabián Rosales-Ortega0Instituto Nacional de Astrofísica, Óptica y Electrónica, Luis E. Erro 1, 72840 Tonantzintla, PUE, MexicoA new generation of wide-field emission-line surveys based on integral field units (IFU) is allowing us to obtain spatially resolved information of the gas-phase emission in nearby late-type galaxies, based on large samples of HII regions and full two-dimensional coverage. These observations are allowing us to discover and characterise abundance differentials between galactic substructures and new scaling relations with global physical properties. Here I review some highlights of our current studies employing this technique: (1) the case study of NGC 628, the largest galaxy ever sampled with an IFU; (2) a statistical approach to the abundance gradients of spiral galaxies, which indicates a universal radial gradient for oxygen abundance; and (3) the discovery of a new scaling relation of HII regions in spiral galaxies, the local mass-metallicity relation of star-forming galaxies. The observational properties and constrains found in local galaxies using this new technique will allow us to interpret the gas-phase abundance of analogue high-z systems.http://dx.doi.org/10.1155/2013/627867
spellingShingle Fernando Fabián Rosales-Ortega
The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era
Advances in Astronomy
title The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era
title_full The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era
title_fullStr The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era
title_full_unstemmed The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era
title_short The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era
title_sort study of nebular emission on nearby spiral galaxies in the ifu era
url http://dx.doi.org/10.1155/2013/627867
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