FUSE and IUE Measurements of D, N, O, and H Toward LSE 44

Details FUSE and IUE Measurements of D, N, O, and H Toward LSE 44 FUSE and IUE Measurements of D, N, O, and H Toward LSE 44

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..348...79f&link_type=abstract

Astrophysics in the Far Ultraviolet: Five Years of Discovery with FUSE ASP Conference Series, Vol. 348, Proceedings of the Confe

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present an analysis of the sight line toward LSE 44, an sdO star located just beyond the Local Bubble. We derive D I, O I, N I, H I and H2 column densities, and the H2 molecular fraction, along this sight line. We find that the D/O and D/N ratios are similar to those along other distant sight lines, but the D/H, O/H and N/H ratios are approximately a factor of 3 higher than typical.

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