Sustaining a Warm Corona in Active Galactic Nuclei Accretion Discs

Abstract

Warm coronae, thick (${\tau }_{\mathrm{T}}\approx 10$-$20$, where ${\tau }_{\mathrm{T}}$ is the Thomson depth) Comptonizing regions with temperatures of $\sim 1$ keV, are proposed to exist at the surfaces of accretion discs in active galactic nuclei (AGNs). By combining with the reflection spectrum, warm coronae may be responsible for producing the smooth soft excess seen in AGN X-ray spectra. This paper studies how a warm corona must adjust in order to sustain the soft excess through large changes in the AGN flux. Spectra from one-dimensional constant density and hydrostatic warm coronae models are calculated assuming the illuminating hard X-ray power-law, gas density, Thomson depth and coronal heating strength vary in response to changes in the accretion rate. We identify models that produce warm coronae with temperatures between $0.3$ and $1.1$ keV, and measure the photon indices and emitted fluxes in the $0.5$-$2$ keV and $2$-$10$ keV bands. Correlations and anti-correlations between these quantities depend on the evolution and structure of the warm corona. Tracing the path that an AGN follows through these correlations will constrain how warm coronae are heated and connected to the accretion disc. Variations in the density structure and coronal heating strength of warm coronae will lead to a variety of soft excess strengths and shapes in AGNs. A larger accretion rate will, on average, lead to a warm corona that produces a stronger soft excess, consistent with observations of local Seyfert galaxies.

12 pages, 8 figures, accepted by MNRAS

References in corpus (11)

• BAT AGN Spectroscopic Survey - V. X-ray properties of the Swift/BAT 70-month AGN catalog
• Piecing Together the X-ray Background: Bolometric Corrections for Active Galactic Nuclei
• CAIXA: a Catalogue of AGN In the XMM-Newton Archive I. Spectral analysis
• Properties of AGN coronae in the NuSTAR era II: hybrid plasma
• Radiation spectra of warm and optically thick coronae in AGN
• The soft X-ray excess: NLS1s vs. BLS1s
• NuSTAR/XMM-Newton monitoring of the Seyfert 1 galaxy HE 1143-1810. Testing the two-corona scenario
• Examining the Physical Conditions of a Warm Corona in Active Galactic Nuclei Accretion Discs
• X-ray time lags in PG 1211+143
• Ionised Accretion Discs in Active Galactic Nuclei: The Effects of a Lamppost with a Variable Height
• Observations of X-ray reverberation around black holes

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