---
author:
- 'D. Cormier'
- 'V. Lebouteiller'
- 'S. C. Madden'
- 'N. Abel'
- 'S. Hony'
- 'F. Galliano'
- 'M. Baes'
- 'M. J. Barlow'
- 'A. Cooray'
- 'I. De Looze'
- 'M. Galametz'
- 'O. Ł. Karczewski'
- 'T. J. Parkin'
- 'A. R[é]{}my'
- 'M. Sauvage'
- 'L. Spinoglio'
- 'C. D. Wilson'
- 'R. Wu'
bibliography:
- '../../BIB/references.bib'
title: ' The nature of the interstellar medium of the starburst low-metallicity galaxy Haro11: a multi-phase model of the infrared emission [^1] '
---

[The low metallicity interstellar medium (ISM) is profoundly different from that of normal systems, being clumpy with low dust abundance and little CO-traced molecular gas. Yet many dwarf galaxies in the nearby universe are actively forming stars. As the complex ISM phases are spatially mixed with each other, detailed modeling is needed to understand the gas emission and subsequent composition and structure of the ISM.]{} [Our goal is to describe the multi-phase ISM of the infrared bright low-metallicity galaxy Haro11, dissecting the photoionised and photodissociated gas components.]{} [We present observations of the mid-infrared and far-infrared fine-structure cooling lines obtained with the [*Spitzer*]{}/IRS and [*Herschel*]{}/PACS spectrometers. We use the spectral synthesis code 