Other
Scientific paper
May 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...190.2506d&link_type=abstract
American Astronomical Society, 190th AAS Meeting, #25.06; Bulletin of the American Astronomical Society, Vol. 29, p.807
Other
Scientific paper
The UV-bright star Barnard 29 in the globular cluster M13 was observed for a total of 8000 seconds with the Berkeley EUV/FUV spectrometer during the ORFEUS-II space-shuttle mission in 1996 November. The resulting spectrum extends from the interstellar cutoff at 912 Angstroms to ~ 1216 Angstroms at a resolution of ~ 0.3 Angstroms. It shows numerous absorption features, but no significant emission features other than terrestrial airglow lines. We present a preliminary analysis of the stellar spectrum, including estimates of its atmospheric parameters and chemical composition derived from LTE and non-LTE stellar atmosphere modeling and spectral synthesis. This work is supported by NASA grant NAG5-696.
Dixon William V.
Hurwitz Margaret M.
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