High Dispersion Observations of the Central Star of NGC 7293

Physics

Scientific paper

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Scientific paper

Preliminary, short exposures of the central star of NGC 7293 by Kudritzki et al. during the 6th year episode of IUE indicate that in addition to photospheric features of C IV and N V, a large number of Fe VI lines were observed. These observations were, however, not of sufficient length to obtain the desired signal to noise ratios, and we would therefore like to obtain a combined 16 hr SWP spectrogram to be started al; Vilspa and then to be finished at GSFC.

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