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Observing ultraviolet signatures of interstellar organics with the Hubble Space Telescope

Published online by Cambridge University Press:  01 February 2008

Theodore P. Snow*
Affiliation:
Center for Astrophysics and Space Astronomy, University of Colorado389 UCBBoulder, CO 80309-0389U.S.A. e-mail: [email protected]
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Abstract

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The Cosmic Origins Spectrograph (COS) will be more sensitive for ultraviolet spectroscopy than either the GHRS or the STIS, especially in the far UV where many absorption lines and bands formed by atoms and molecules have electronic transitions from the ground state. Here we outline our plans for using the COS to observe interstellar gas and dust in the cold ISM, along with a report on the results of preliminary archival HST search for UV diffuse interstellar bands.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

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