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S. Bowyer
Center for EUV Astrophysics, 2150 Kittredge Street, University
of California, Berkeley, CA 94720
Observations in the EUV band have provided new insights into the interstellar medium. In the following I discuss two areas in which EUV observations are providing unique information: the ionization state of the ISM, and the pressure of the hot phase of the local interstellar medium and the bearing of this work on the McKee-Ostriker model of the ISM.
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