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Determination of Velocity and Radius of Supernova Remnant after 1000 yrs of Explosion 被引量:1

Determination of Velocity and Radius of Supernova Remnant after 1000 yrs of Explosion
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摘要 Supernova explosions are described as very violent events which transfer a significant amount of energy to interstellar media and are responsible for a large variety of physical processes. This study does not discuss the actual explosion mechanisms but follows the behavior of the dynamical evolution of some selected type I and type II supernova remnant and particularly after a thousand years from their explosion and shows how the density of the medium affects the evolution and the lifetime of each remnant. By studying such behaviors, a simplified model has been proposed here for the velocity and radius of the remnant after thousand years of explosion that depends only on the density of the medium and age of the remnant. It has been found that all types of supernova remnants have similar behaviors after a thousand years from their explosion despite their origin formation. Moreover, it is demonstrated that, when those selected remnants have entered or will enter into their radiative phase, an idea on their physical properties will be obtained. Supernova explosions are described as very violent events which transfer a significant amount of energy to interstellar media and are responsible for a large variety of physical processes. This study does not discuss the actual explosion mechanisms but follows the behavior of the dynamical evolution of some selected type I and type II supernova remnant and particularly after a thousand years from their explosion and shows how the density of the medium affects the evolution and the lifetime of each remnant. By studying such behaviors, a simplified model has been proposed here for the velocity and radius of the remnant after thousand years of explosion that depends only on the density of the medium and age of the remnant. It has been found that all types of supernova remnants have similar behaviors after a thousand years from their explosion despite their origin formation. Moreover, it is demonstrated that, when those selected remnants have entered or will enter into their radiative phase, an idea on their physical properties will be obtained.
出处 《International Journal of Astronomy and Astrophysics》 2015年第2期125-132,共8页 天文学与天体物理学国际期刊(英文)
关键词 SUPERNOVA SUPERNOVA REMNANT RADIATIVE PHASE Supernova Supernova remnant Radiative Phase
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  • 1Leonard Wegert,Stephan Schreiner,Constantin Rauch,Bruno Albertazzi,Paulina Bleuel,Eric Frojdh,Michel Koenig,Veronika Ludwig,Artem SMartynenko,Pascal Meyer,Aldo Mozzanica,Michael Müller,Paul Neumayer,Markus Schneider,Angelos Triantafyllidis,Bernhard Zielbauer,Gisela Anton,Thilo Michel,Stefan Funk.Demonstrating grating-based phase-contrast imaging of laser-driven shock waves[J].Matter and Radiation at Extremes,2024,9(4):90-97.

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