Spectral Analysis of Super Soft X-ray Sources: V4743 Sagittarii
Astrophysics
2007-05-23 v1
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 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.
Keywords
Cite
@article{arxiv.astro-ph/0410700,
title = {Spectral Analysis of Super Soft X-ray Sources: V4743 Sagittarii},
author = {Thomas Rauch and Marina Orio and R. Gonzales-Riestra and Martin Still},
journal= {arXiv preprint arXiv:astro-ph/0410700},
year = {2007}
}
Comments
4 pages, 3 figure, proceedings "14th European Workshop on White Dwarfs", Jul 2004, Kiel, Germany