The Interstellar Medium in the Far Ultraviolet

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Interstellar Medium And Nebulae In External Galaxies, Magellanic Stream, Astronomical Observations

Scientific paper

During its lifetime, FUSE produced a broad array of exciting results on the interstellar medium (ISM) of our own Milky Way and other galaxies. Some of its most important contributions in this area are in the physics of the highly ionized gas traced by O VI and of the molecular medium traced by the Lyman and Werner bands of H2. I briefly note a few of these successes and discuss future directions and wishes for studying the ISM with next generation instruments.

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