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• W3105147843 abstract "We analyze the Chandra X-ray spectrum obtained with the HETGS grating spectrometer of IRAS 13349+2438, which has one of the richest absorption spectra of a quasar outflow. Absorption from almost all charge states of Fe is detected. This allows for a detailed reconstruction of the absorption measure distribution (AMD), which we define as the continuous distribution of column density as a function of ionization parameter. We find a double peaked AMD for IRAS 13349+2438 with a total (ionized) column density of N_H = (1.2 +- 0.3)* 10^{22} cm^-2} assuming solar iron abundance. For comparison, we perform a similar analysis on the well studied HETGS spectrum of NGC 3783. Both sources feature a deep minimum in column density consistent with no absorption from gas at temperatures of 4.5 < log T < 5 (K). We interpret the minima as observational evidence for thermal instability in this temperature regime." @default.
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• W3105147843 date "2007-07-10" @default.
• W3105147843 modified "2023-09-29" @default.
• W3105147843 title "Absorption Measure Distribution of the Outflow in IRAS 13349+2438: Direct Observation of Thermal Instability?" @default.
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• W3105147843 doi "https://doi.org/10.1086/518416" @default.
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