Non-equilibrium x-ray emission from young supernova remnants
Thesis/Dissertation
·
OSTI ID:5008838
A computer model (NIE model) has been developed to predict the x-ray spectra from the hot (10/sup 6 -8/K), shock-heated plasmas that are found in the remnants of supernovae. The model accounts for the lack of collisional ionization equilibrium and for the possible lack of thermal equilibrium between the electrons and ions behind the shock fronts. Both of these effects are potentially important in determining the emergent x-ray spectrum of young (
- Research Organization:
- California Inst. of Tech., Pasadena (USA)
- OSTI ID:
- 5008838
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640103* -- Astrophysics & Cosmology-- Quasi-Stellar
Radio
& X-Ray Sources-- (-1987)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COMPUTERIZED SIMULATION
COSMIC RADIO SOURCES
EQUILIBRIUM
INTERSTELLAR SPACE
PLASMA
SHOCK WAVES
SIMULATION
SPACE
SPECTRA
SUPERNOVA REMNANTS
THERMAL EQUILIBRIUM
X-RAY SPECTRA
Radio
& X-Ray Sources-- (-1987)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COMPUTERIZED SIMULATION
COSMIC RADIO SOURCES
EQUILIBRIUM
INTERSTELLAR SPACE
PLASMA
SHOCK WAVES
SIMULATION
SPACE
SPECTRA
SUPERNOVA REMNANTS
THERMAL EQUILIBRIUM
X-RAY SPECTRA