A New Ionization Balance for Optically Thin Plasmas: the Implication for the Calculated X Ray Spectrum.

Details A New Ionization Balance for Optically Thin Plasmas: the Implication for the Calculated X Ray Spectrum. A New Ionization Balance for Optically Thin Plasmas: the Implication for the Calculated X Ray Spectrum.

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.525m&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

The next coming X ray mission will allow us to measure the emission of the astrophysical X-ray sources with high energy resolution. Nevertheless to determine the relevant physical parameters describing the plasmas we need to compare observed data with a t This year we developed a new ionization balance code. This code as been already included in the spectral code SPEX. In this paper we show how the result of the standard analysis of AXAF or XMM spectra could be affected by the use of different ionization b

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