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

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

2004-10-28

arxiv.org/abs/astro-ph/0410700v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figure, proceedings "14th European Workshop on White Dwarfs", Jul 2004, Kiel, Germany

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Spectral Analysis of Super Soft X-ray Sources: V4743 Sagittarii does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectral Analysis of Super Soft X-ray Sources: V4743 Sagittarii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral Analysis of Super Soft X-ray Sources: V4743 Sagittarii will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-344757