Statistics – Computation
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.228..453d&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 228, Sept. 15, 1987, p. 453-461.
Statistics
Computation
24
Background Radiation, Magnetohydrodynamic Flow, Mass Flow, Stellar Structure, Supernova Remnants, X Ray Astronomy, Computational Astrophysics, Gas Flow, Similarity Theorem
Scientific paper
A similarity solution for a supernova remnant whose mass is dominated by material mixed in by hydrodynamic ablation from embedded clumps of gas is derived. This solution is used to calculate the properties of a remnant which can reproduce both the relative and absolute count rates in the M, B, and C soft X-ray bands measured for the local supernova remnant. It is also shown that it is possible to produce the same soft X-ray counts in a remnant whose mass is dominated by material injected by conductive mixing. The global properties of the remnants are remarkably similar in both cases. It is concluded that it is not possible to distinguish uniquely between physically very different remnant structures on the basis of soft X-ray counts alone.
Dyson John E.
Hartquist Thomas W.
No associations
LandOfFree
Mass loaded astronomical flows. III - The structure of supernova remnants and the local soft X-ray background 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 Mass loaded astronomical flows. III - The structure of supernova remnants and the local soft X-ray background, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass loaded astronomical flows. III - The structure of supernova remnants and the local soft X-ray background will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1676559