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The Universe as Seen by ISO

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The article was published on 1999-03-01 and is currently open access. It has received 767 citations till now. The article focuses on the topics: Luminous infrared galaxy.

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Journal ArticleDOI

Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era

TL;DR: In this paper, the authors calculated IR emission spectra for dust heated by starlight, for mixtures of amorphous silicate and graphitic grains, including varying amounts of PAH particles.
Journal ArticleDOI

Infrared Emission from Interstellar Dust. II. The Diffuse Interstellar Medium

TL;DR: In this article, the authors present a quantitative model for the infrared emission from dust in the diffuse interstellar medium, which consists of a mixture of amorphous silicate grains and carbonaceous grains, each with a wide size distribution ranging from molecules containing tens of atoms to large grains 1 μm in diameter.
Journal ArticleDOI

Neutral Atomic Phases of the Interstellar Medium in the Galaxy

TL;DR: In this paper, the authors provided an analytic approximation for Pmin as a function of metallicity, far-ultraviolet radiation field, and the ionization rate of atomic hydrogen.
Journal ArticleDOI

The Dust Opacity of Star‐forming Galaxies

TL;DR: In this article, a review of existing theoretical and empirical measures of opacity in local galaxies are reviewed together with widely used theoretical and empirically derived methods for quantifying its effects, and a digression is devoted to starbursts in view of their potential relevance for measure of opacity.
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