Dust properties and distribution in dwarf galaxies Lisenfeld , Ute Relaño Pastor, Mónica Vílchez, José Battaner López, Eduardo Hermelo, Israel ISM Dust Galaxies ISM NGC 1569 NGC 4214 Dwarf 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. 2013-10-09T12:22:57Z 2013-10-09T12:22:57Z 2008 info:eu-repo/semantics/preprint 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] 1743-9213 1743-9221 arXiv:0808.1953v1 http://hdl.handle.net/10481/28394 10.1017/S1743921308024915 eng http://creativecommons.org/licenses/by-nc-nd/3.0/ info:eu-repo/semantics/openAccess Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License Cambridge University Press; International Astronomical Union (IAU)