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- W2009793844 abstract "Here we review some of our more recent results on the observed properties of H II regions using Integral Field Spectroscopy. In particular, we illustrate the use of this technique to study in detail the ionization conditions across the nebulae for galactic H II regions (focused on the Orion Nebula) and the statistical study of large samples of extragalactic H II regions. We review the reported new scaling relation between the local mass density and the oxygen abundance across the disk galaxies and the recently discovered universal gradient for oxygen abundances. We update our previous results the lack of a dependence of the Mass-Metallicity relation with the starformation rate, including new unpublished data. Finally we discuss on the relation between the ionization conditions in the nebulae and the underlying stellar population. All together our results indicate that disk galaxies present a chemical enrichment dominated by an inside-out growth scenario, with a less evident effect of radial migrations and/or outflows." @default.
- W2009793844 created "2016-06-24" @default.
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- W2009793844 date "2013-01-01" @default.
- W2009793844 modified "2023-10-17" @default.
- W2009793844 title "Properties of the HII Regions Derived Using Integral Field Spectroscopy" @default.
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- W2009793844 doi "https://doi.org/10.1155/2013/596501" @default.
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