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- W1569488904 abstract "At high redshift the ubiquity of outflows and winds in strongly star-forming galaxies has been demonstrated using rest frame UV absorption lines. In the cases with optical emission lines, the studies mostly had to rely on low and intermediate dispersion spectra. This implies that for detailed studies of galactic wind physics we have to use local objects. In particular, dwarf galaxies are well suited to extrapolation to high redshift protogalaxies. Several kinematic studies of strongly starforming dwarf galaxies using Fabry-Perot and IFU spectrographs exist. Unfortunately, similar as for high redshift galaxies the employed spectral resolution is often significantly higher that the thermal line width. As a result faint high velocity features and details of the turbulent motion are hidden or unresolved. Here we will present an analysis of the ionized gas kinematics of the prototypical star-forming irregular galaxy NGC 4449 using long-slit, high-dispersion echelle spectra. (© 2014 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)" @default.
- W1569488904 created "2016-06-24" @default.
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- W1569488904 date "2014-01-01" @default.
- W1569488904 modified "2023-10-14" @default.
- W1569488904 title "Long-slit échelle spectroscopy of galactic outflows: The case ofNGC 4449" @default.
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- W1569488904 doi "https://doi.org/10.1002/asna.201312019" @default.
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