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Far- to near-UV spectroscopy of the interstellar medium at very high resolution and very high signal-to-noise ratio

Published onMay 31, 2019
Far- to near-UV spectroscopy of the interstellar medium at very high resolution and very high signal-to-noise ratio
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Abstract

A comprehensive study of the ISM phases and the nature of their connections requires comparing abundances and velocity profiles of tracers of the different phases. A wealth of absorption features from such tracers are found in the full UV domain that need to be observed at high resolving power R > 200 000 and high signal-to-noise ratio SNR > 500.

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