ORFEUS-II Observations of the Ultraviolet-Bright Star Barnard 29 in M13

Details ORFEUS-II Observations of the Ultraviolet-Bright Star Barnard 29 in M13 ORFEUS-II Observations of the Ultraviolet-Bright Star Barnard 29 in M13

1998-04-15

arxiv.org/abs/astro-ph/9804147v1

Astronomy and Astrophysics

Astrophysics

LaTeX file, 6 pages, 3 encapsulated PostScript figures. Uses aas2pp4.sty and astrobib.sty. (Astrobib is available from http:

Scientific paper

10.1086/311391

The UV-bright star Barnard 29 in the globular cluster M13 was observed for 5300 seconds with the Berkeley spectrometer on the ORFEUS-SPAS II Mission in 1996 November-December. The resulting spectrum extends from the interstellar cutoff at 912 A to ~ 1200 A at a resolution of ~ 0.33 A. It shows numerous absorption features, both photospheric and interstellar, but no significant emission other than diffuse emission of local origin. The Kurucz synthetic stellar spectrum that best fits the data has T_eff = 21,000 K, log g = 3.0, and [M/H] = -2.5. This effective temperature and surface gravity are consistent with previous results, but the derived metallicity is lower than that of other M13 giants, for which [Fe/H] = -1.60. Using high-resolution synthetic spectra, we determine the photospheric abundances of C, S, and Fe, species unobservable in the optical. We find log epsilon(C) = 6.15 +/- 0.10, log epsilon(S) = 5.34 +/- 0.50, and log epsilon(Fe) = 5.30 (+0.22, -0.26). Again, the Fe abundance is lower than expected. This anomaly may reflect selective condensation of metals onto dust grains at the end of the AGB phase, as has been suggested for some cooler post-AGB stars with peculiar Fe abundances.

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