Uv Spectroscopic Determination of the D/h Ratio Along the Line of Sight Toward Epsilon-Ind and Lambda-And

Details Uv Spectroscopic Determination of the D/h Ratio Along the Line of Sight Toward Epsilon-Ind and Lambda-And Uv Spectroscopic Determination of the D/h Ratio Along the Line of Sight Toward Epsilon-Ind and Lambda-And

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5650a&link_type=abstract

HST Proposal ID #5650

Physics

Hst Proposal Id #5650 Ism

Scientific paper

The HST will be used to obtain high-resolution UV spectra of the lines of sight toward Epsilon-Ind and Lambda-And. These lines of sight were previously observed by earlier instruments. The Goddard High Resolution Spectrograph will make the D/H values toward these lines of sight much more reliable. Thus, the D/H value for the Local Interstellar Medium (LISM) will be known with much more accuracy. This is a crucial measure- ment needed to determine the Baryon/Photon ratio and hence the ultimate fate of the universe.

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