Spectral Analysis of Super Soft X-ray Sources: V4743 Sagittarii

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dc.creatorRauch, Thomas
dc.creatorOrio, Marina
dc.creatorGonzales-Riestra, R.
dc.creatorStill, Martin
dc.date2004-10-28
dc.date.accessioned2026-07-07T02:15:33Z
dc.date.available2026-07-07T02:15:33Z
dc.descriptionHalf 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 30A, exhibiting resonance lines of C V, C VI, N VI, N VII, and O VII. We present preliminary results of an analysis of the XMM-Newton RGS spectra by means of NLTE model-atmosphere techniques.
dc.description4 pages, 3 figure, proceedings "14th European Workshop on White Dwarfs", Jul 2004, Kiel, Germany
dc.identifierhttps://arxiv.org/abs/astro-ph/0410700
dc.identifierhttp://arxiv.org/abs/astro-ph/0410700
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8451
dc.subjectAstrophysics
dc.titleSpectral Analysis of Super Soft X-ray Sources: V4743 Sagittarii
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