Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...167..120r&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 167, no. 1, Oct. 1986, p. 120-128.
Astronomy and Astrophysics
Astrophysics
10
Collisions, Interstellar Matter, Mach Reflection, Supernova Remnants, Adiabatic Conditions, Radiant Cooling, Two Dimensional Models
Scientific paper
High-resolution, two-dimensional models of colliding supernova remnants in a dense (n = 103cm-3) medium are presented. The paper is focussed on hydrodynamical phenomena taking place in the vicinity of the interaction plane. Reflected shocks and Mach disks form there, and the gas swept by them evolves into a dense ring moving along the interaction plane ahead of the main supernova shock. The ring is of transient nature in adiabatic remnants, but when allowances for radiative cooling are made it persists for some time. The calculations provide a feasible explanation for the origin of certain anomalous H I velocity features and morphological peculiarities observed in supernova remnants.
Bodenheimer Peter
Rozyczka Michal
Tenorio-Tagle Guillermo
No associations
LandOfFree
Non-spherical supernova remnants. III - Oblique shock reflections and anomalous H I velocity features 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 Non-spherical supernova remnants. III - Oblique shock reflections and anomalous H I velocity features, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-spherical supernova remnants. III - Oblique shock reflections and anomalous H I velocity features will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1735052