The status and future of EUV astronomy |
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| Authors: | M.A. Barstow S.L. Casewell J.B. Holberg M.P. Kowalski |
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| Affiliation: | 1. Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK;2. Lunar and Planetary Laboratory, 1541 East University Boulevard, Sonett Space Sciences Building, University of Arizona, Tucson, AZ 85721, USA;3. Naval Research Laboratory, 4555 Overlook Ave SW, Washington, DC 20375, USA |
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| Abstract: | The Extreme Ultraviolet wavelength range was one of the final windows to be opened up to astronomy. Nevertheless, it provides very important diagnostic tools for a range of astronomical objects, although the opacity of the interstellar medium restricts the majority of observations to sources in our own galaxy. This review gives a historical overview of EUV astronomy, describes current instrumental capabilities and examines the prospects for future facilities on small and medium-class satellite platforms. |
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| Keywords: | Extreme Ultraviolet Spectroscopy White dwarfs Stellar coronae Interstellar medium |
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