Please use this identifier to cite or link to this item:
|Title:||The status and future of EUV astronomy|
|Authors:||Barstow, M. A.|
Casewell, S. L.
Holberg, J. B.
Kowalski, M. P.
|Publisher:||Elsevier for Committee on Space Research (COSPAR), Pergamon|
|Citation:||Advances in Space Research, 2014, 53 (6), pp. 1003-1013 (11)|
|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.|
|Rights:||Creative Commons “Attribution Non-Commercial No Derivatives” licence CC BY-NC-ND, further details of which can be found via the following link: http://creativecommons.org/licenses/by-nc-nd/4.0/ Archived with reference to SHERPA/RoMEO and publisher website.|
|Appears in Collections:||Published Articles, Dept. of Physics and Astronomy|
Files in This Item:
|1309.2181v1.pdf||Post-review (final submitted author manuscript)||1.75 MB||Adobe PDF||View/Open|
Items in LRA are protected by copyright, with all rights reserved, unless otherwise indicated.