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Observations of Local ISM Emission With the Berkeley EUV/FUV Shuttle Telescope

Published online by Cambridge University Press:  12 April 2016

Christopher Martin  and
Stuart Bowyer
Christopher Martin
Affiliation:
Space Science Laboratory, University of California, Berkeley
Stuart Bowyer
Affiliation:
Space Science Laboratory, University of California, Berkeley

Abstract

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The Berkeley Extreme Ultraviolet/Far Ultraviolet Shuttle Telescope (BEST) will be launched on the Space Shuttle in November, 1984, as part of the NASA UVX project. The Berkeley spectrometer will make observations of the cosmic diffuse background in the 600-1900 Å band, with a spectral resolution of 10 Å. The sensitivity and spectral resolution of the instrument make it ideal for the study of components of the interstellar medium in the 104 - 106K range.

Type
Things To Come
Information
International Astronomical Union Colloquium , Volume 81: Local Interstellar Medium , 1984 , pp. 344 - 347
Copyright
Copyright © NASA 1984

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