Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-06-09
Astrophys.J. 542 (2000) 684
Astronomy and Astrophysics
Astrophysics
21 pages including 8 figures and 4 tables; accepted for publication to the Astrophysical Journal
Scientific paper
10.1086/317053
We present a detailed X-ray spectral analysis of the Circinus Galaxy using archival data obtained with the ASCA satellite. The spectrum shows numerous emission lines in the soft X-ray band from highly ionized ions, as well as Compton reflection and fluorescent lines from neutral or near-neutral matter. We analyze the spectrum in the context of a self-consistent recombination cascade model and find that a nearly flat differential emission measure (DEM) distribution in ionization parameter fits the data. For a fixed solid angle distribution of matter surrounding a point source, this corresponds to a run of electron density of the form, n(r) ~ r^(-3/2), which is suggestive of Bondi accretion onto a central compact mass. Using this density profile and comparing the resulting emission spectra with the ASCA data, the size of the X-ray emission line region is estimated to be < 1 kpc. We also show that the derived density as a function of radius is compatible with the X-ray recombination line emission region being the confining medium of the coronal line regions.
Kahn Steven M.
Liedahl Duane Allen
Paerels Frits
Sako Masao
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