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• W5232579 abstract "We analyze the full bi-dimensional spectral cube of the nearby spiral galaxy NGC 5668, which was obtained as a mosaic of 6 pointings, covering a total area of 2× 3 arcmin2, obtained with the PPAK Integral Field Unit at the Calar Alto (CAHA) observatory 3.5 m telescope. From these data we derive maps of the attenuation of the ionized gas (from the Hα / Hβ Balmer decrement), electron density (from the [SII]6717A/ [SII]6731A ratio), and chemical abundances, of both oxygen (using either the Te based method when possible or strong line methods such as the R23), and nitrogen. In addition to these maps, we also extract the spectra of individual HII regions by adding the flux over several PPAK fibers to increase the signal-to-noise ratio of the spectra and reduce the uncertainties in the properties derived. Along with the study of the ionized gas we also embark in the analysis of the absorption-line spectrum dominating the bulge and inter-arm regions. The spectra of these regions are compared with the predictions of evolutionary synthesis models for evolved stellar populations. Both the measurements of spectroscopic indices and the full spectra will be used. Finally, given that most of the properties of the stars, gas, and dust in galaxies vary with radius; the spectra of concentric annuli are also extracted and analyzed." @default.
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• W5232579 date "2010-01-01" @default.
• W5232579 modified "2023-09-24" @default.
• W5232579 title "Integral Field Spectroscopy of the nearby spiral galaxy NGC 5668" @default.
• W5232579 hasPublicationYear "2010" @default.
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