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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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