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Please use this identifier to cite or link to this item: http://hdl.handle.net/10481/28394

Title: Dust properties and distribution in dwarf galaxies
Authors: Lisenfeld, Ute
Relaño, Mónica
Vílchez, José
Battaner, E.
Hermelo, Israel
Issue Date: 2008
Abstract: We present a study of the extinction, traced by the Balmer decrement, in HII regions in the dwarf galaxies NGC 1569 and NGC 4214. We find that the large-scale extinction around the most prominent HII regions in both galaxies forms a shell in which locally the intrinsic extinction can adopt relatively high values ($A_V = 0.8 - 0.9$ mag) despite the low metallicity and thus the low overall dust content. The small-scale extinction (spatial resolution $\sim$0.3'') shows fluctuations that are most likely due to variations in the dust distribution. We compare the distribution of the extinction to that of the dust emission, traced by Spitzer emission at 8 and 24 \mi, and to the emission of cold dust at 850 \mi. We find in general a good agreement between all tracers, expect for the 850 \mi emission in NGC 4214 which is more extended than the extinction and the other emissions. Whereas in NGC 1569 the dust emission at all wavelengths is very similar, NGC 4214 shows spatial variations in the 24-to-850 \mi ratio. We furthermore compared the 24 \mi and the extinction-corrected Halpha emission from HII regions in a sample of galaxies with a wide range of metallicities and found a good correlation between both emissions, independent of metallicity. We suggest that this lack of dependence on metallicity might be due to the formation of dust shells with a relatively constant opacity, like the ones observed here, around ionizing stars.
Publisher: Cambridge University Press; International Astronomical Union (IAU)
Keywords: ISM
NGC 1569
NGC 4214
URI: http://hdl.handle.net/10481/28394
ISSN: 1743-9213
Rights : Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License
Citation: Lisenfeld, U.; et al. Dust properties and distribution in dwarf galaxies. Proceedings of the International Astronomical Union, 4(S255): 260-264 (2008). [http://hdl.handle.net/10481/28394]
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