HIGHLIGHTS
- who: Polles F. L. and colleagues from the Laboratoire AIM, CEA/Service d'Astrophysique, Bât709, CEA-Saclay, Gif-sur-Yvette , France, CNRS, PSL University, Sorbonne University, France have published the Article: Modeling ionized gas in low-metallicity environments: the Local Group dwarf galaxy IC, in the Journal: (JOURNAL)
- what: The mid- and far-infrared (MIR and FIR) lines - the focus of this paper - are less affected by the dust and gas attenuation compared to optical lines, and are therefore potentially ideal tracers of the ISM parameters deeper into star forming clouds. In Fig 5 . . .
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