Theoretical study of the X-ray emission from astrophysical shock waves

Details Theoretical study of the X-ray emission from astrophysical shock waves Theoretical study of the X-ray emission from astrophysical shock waves

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sao..rept.....r&link_type=abstract

Semiannual Report, 1 Jun. 1985 - 31 May 1986 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Cataclysmic Variables, Mathematical Models, Photoionization, Shock Waves, Stellar Winds, Supernovae, Time Dependence, X Ray Spectra, Cooling, Emission Spectra, Energy Bands, Line Spectra

Scientific paper

Theoretical X-ray emission spectra are needed to interpret the X-ray emission observed by many low and moderate resolution X-ray instruments, and to provide diagnosis of physical conditions for high resolution spectra. Over the past decade, a set of model codes which compute the X-ray and XUV emission for a wide set of physical conditions, including high or low densities, photoionized gas, and time-dependent ionization balance was developed. In the past year, the atomic rate coefficients in the code was improved. Further capabilities were added, and applied to several astrophysical problems.

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