The Interstellar Gas toward LSE 234. A High D/H Ratio beyond the Local Bubble

Details The Interstellar Gas toward LSE 234. A High D/H Ratio beyond the Local Bubble The Interstellar Gas toward LSE 234. A High D/H Ratio beyond the Local Bubble

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..348...88l&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

LSE 234 is a sub-dwarf located at about 400 parsecs. We obtained FUSE spectra with very good signal-to-noise ratio, allowing accurate abundance measurements. We find high values for D/H, D/N and D/O in this sight line probing material well beyond the Local Bubble. This is in contrast with published measurements at such distances (Hébrard & Moos 2003, Wood et al. 2004). This favors the hypothesis of D/H inhomogeneities outside the Local Bubble.

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