Abstract
We present the results of a recent spectroscopic investigation of the cool DO white dwarf HD 149499 B in the EUV and FUV ranges. Observations were performed with the spectrograph of the EUVE satellite and the Berkeley EUV/FUV spectrometer of the ORFEUS space experiment.† The analysis of the ORFEUS spectrum, performed with a grid of LTE model atmospheres, yielded the basic parameters T eff = 49500 ± 500 K and log g = 7.97 ± 0.08. This result is confirmed by the EUVE spectra. The photospheric hydrogen Lyman lines in the FUV spectrum indicate the presence of hydrogen: log nH/nHe = -0.65 ± 0.12. The implications of this finding for the spectral evolution of white dwarfs are discussed. A check of the LTE assumption was performed by a comparison with NLTE atmospheres calculated for appropriate parameters. The interstellar hydrogen column towards the HD 149499 system amounts to N H = (7±2)·1018 cm-2.
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© 1996 Springer Science+Business Media Dordrecht
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Napiwotzki, R. et al. (1996). EUVE and ORFEUS Observations of the Cool DO White Dwarf HD 149499 B. In: Bowyer, S., Malina, R.F. (eds) Astrophysics in the Extreme Ultraviolet. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3988-5_39
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DOI: https://doi.org/10.1007/978-94-011-3988-5_39
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