arXiv · astro-ph/0212341
The thin layer of Warm Ionized Gas: towards a 3-D reconstruction of the spatial distribution of HII regions
Abstract
HII regions are known to contribute to the so-called thin layer of the diffuse Warm Ionized Gas. In order to constrain this contribution, we reconstruct the 3-D distribution of the sources. A detailed spatial analysis of the largest up-to-date sample of HII regions is presented.
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Roberta Paladini, Rod Davies, Gianfranco DeZotti. 2002-12-15. The thin layer of Warm Ionized Gas: towards a 3-D reconstruction of the spatial distribution of HII regions. https://doi.org/10.1023/b%3Aastr.0000014983.24270.e5
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