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Paper: Spectral Analysis of Super Soft X-ray Sources: V4743 Sagittarii
Volume: 334, 14th European Workshop on White Dwarfs
Page: 423
Authors: Rauch, T.; Orio, M.; Gonzales-Riestra, R.; Still, M.
Abstract: Half a year after its outburst, the nova V4743 Sgr evolved into the brightest super-soft X-ray source in the sky with a flux maximum around 30 Å, exhibiting resonance lines of CV, CVI, NVI, NVII, and OVII. We present preliminary results of an analysis of the XMM-Newton RGS spectra by means of NLTE model-atmosphere techniques.
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