Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-09-24
Astronomy and Astrophysics
Astrophysics
3 figs. To be published in Proc of Annapolis workshop on magnetic CVs, July 1998
Scientific paper
The post-shock flow in the accretion region of MCVs is considered to be a magnetically confined cooling flow. The X-ray spectrum from this hot plasma is emitted from a range of temperatures and densities. Extracting information from such spectra obtained with the next generation of X-ray satellites will rely on models for the structure of this flow which include appropriate treatment of the cooling mechanisms, boundary conditions and of absorptions and reflection components. This paper summarises the current situation and explores some of the difficulties arising in the exploitation of the line emission from these systems. It concludes by looking at improvements to the models now in the pipeline.
Cropper Mark
Ramsay Gavin
Wu Kinwah
No associations
LandOfFree
Continuum and line emission from post-shockc flows 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 Continuum and line emission from post-shockc flows, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Continuum and line emission from post-shockc flows will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-708786