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- W1528837524 abstract "Thanks to the new generation of X-ray satellites such as Chandra and XMM, high resolution and high sensitivity spectra are available. In particular, for the rst time, the three most intense lines (resonance, intercombination and forbidden) of low charged (low Z) He-like ions are split for non-solar plasmas. We present density, ionizing process and temperature diagnostics, for totally and partially photoionized plasmas, based on ratios of these three lines. These powerful plasma diagnostics could be used for hot astrophysical plasmas such as AGN, starburst galaxies, X-ray binaries, etc. In particular, they could be applied to the Warm Absorbers often seen in Active Galactic Nuclei (Porquet & Dubau 2000), which is an important tool for understanding the central regions of dieren t types of AGN (Seyfert 1 and 2, high and low redshift quasars)." @default.
- W1528837524 created "2016-06-24" @default.
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- W1528837524 date "2000-05-01" @default.
- W1528837524 modified "2023-10-18" @default.
- W1528837524 title "X-RAY PLASMA DIAGNOSTICS FOR TOTALLY AND PARTIALLY PHOTOIONIZED PLASMAS SUCH AS WARM ABSORBERS IN AGN" @default.
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