Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2012-01-26
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
16 pages, 10 figures, Accepted for publication in MNRAS
Scientific paper
The radiation from the central regions of active galactic nuclei, including that from the accretion disk surrounding the black hole, is likely to peak in the extreme ultraviolet $\sim 13 -100 \ev$. However, due to Galactic absorption, we are limited to constraining the physical properties - black hole mass and accretion rate - from what observations we have below $\sim 10 \ev$ or above $\sim 100 \ev$. In this paper we predict the thermal and ionization states of warm absorbers as a function of the shape of the unobservable continuum. In particular we model an accretion disk at $kT_{in} \sim 10 \ev$ and a {\it soft excess} at $kT_{se} \sim 150 \ev$. The warm absorber, which is the highly ionized gas along the line of sight to the continuum, shows signatures in the $\sim 0.3 - 2 \kev$ energy range consisting of numerous absorption lines and edges of various ions, some of the prominent ones being H- and He-like oxygen, neon, magnesium and silicon. We find that the properties of the warm absorber are significantly influenced by the changes in the temperature of the accretion disk, as well as by the strength of the {\it soft excess}, as they affect the optical depth particularly for iron and oxygen. These trends may help develop a method of characterising the shape of the unobservable continuum and the occurrence of warm absorbers.
Chakravorty Susmita
Elvis Martin
Ferland Gary
Kembhavi Ajit K.
Misra Ranjeev
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