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The Future for UV Spectroscopy of the ISM at High Resolution

Published online by Cambridge University Press:  30 March 2016

Edward B. Jenkins*
Affiliation:
Princeton University ObservatoryPrinceton, NJ 08544-1001USA

Abstract

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In the post-HST era, advanced missions for performing UV spectroscopy must excel in many ways. We must not overlook the importance of high wavelength resolution for investigating absorption lines from gas systems in the Galaxy and beyond. We consider here some basic principles on this topic, both scientific and technical.

Type
I. Joint Discussions
Copyright
Copyright © Astronomical Society of Pacific 2005

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