학술논문

Adiabatic supernova expansion into the circumstellar medium
Document Type
Conference
Author
Source
Conference: 101. International Astronomics Union colloquium on interaction of supernova remnants with the interstellar medium, Penticon, Canada, 8 Jun 1987; Other Information: Portions of this document are illegible in microfiche products
Subject
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS SUPERNOVAE
COMPUTERIZED SIMULATION
HYDRODYNAMIC MODEL
ADIABATIC PROCESSES
INTERSTELLAR SPACE
MASS DISTRIBUTION
NUMERICAL SOLUTION
SHOCK WAVES
DISTRIBUTION
ERUPTIVE VARIABLE STARS
MATHEMATICAL MODELS
PARTICLE MODELS
SIMULATION
SPACE
SPATIAL DISTRIBUTION
STARS
STATISTICAL MODELS
THERMODYNAMIC MODEL
VARIABLE STARS 640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Radio & X-Ray Sources
Language
English
Abstract
We perform one dimensional numerical simulations with a Lagrangian hydrodynamics code of the adiabatic expansion of a supernova into the surrounding medium. The early expansion follows Chevalier's analytic self-similar solution until the reverse shock reaches the ejecta core. We follow the expansion as it evolves towards the adiabatic blast wave phase. Some memory of the earlier phases of expansion is retained in the interior even when the outer regions expand as a blast wave. We find the results are sensitive to the initial configuration of the ejecta and to the placement of gridpoints. 6 refs., 2 figs.