Modeling of Photoionized Plasmas
arXiv:1009.4663 · doi:10.1007/s11214-010-9711-6
Abstract
In this paper I review the motivation and current status of modeling of plasmas exposed to strong radiation fields, as it applies to the study of cosmic X-ray sources. This includes some of the astrophysical issues which can be addressed, the ingredients for the models, the current computational tools, the limitations imposed by currently available atomic data, and the validity of some of the standard assumptions. I will also discuss ideas for the future: challenges associated with future missions, opportunities presented by improved computers, and goals for atomic data collection.
17 pages, 8 figures, to appear in the proceedings of Xray2010, Utrecht, the Netherlands, March 15-17 2010
References in corpus (4)
- Atomic Data for X-ray Astrophysics
- Multi-dimensional modelling of X-ray spectra for AGN accretion-disk outflows
- An axisymmetric hydrodynamical model for the torus wind in AGN. II: X-ray excited funnel flow
- Thermal instability in X-ray photoionized media in Active Galactic Nuclei: Influence on the gas structure and spectral features
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- Multiphase AGN winds from X-ray irradiated disk atmospheres
- Multi-wavelength campaign on NGC 7469: III. Spectral energy distribution and the AGN wind photoionisation modelling, plus detection of diffuse X-rays from the starburst with Chandra HETGS
- Irradiation of Astrophysical Objects - SED and Flux Effects on Thermally Driven Winds
- Dynamical thermal instability in highly supersonic outflows
- X-ray ionization of the intergalactic medium by quasars
- K-shell photoionization of Be-like Boron (B) Ions: Experiment and Theory
- Absolute rate coefficients for photorecombination and electron-impact ionization of magnesium-like iron ions from measurements at a heavy-ion storage ring
- Low energy range dielectronic recombination of Fluorine-like Fe17+ at the CSRm
- Absolute rate coefficients for photorecombination of berylliumlike and boronlike silicon ions
- Discovery of Red-shifted He-like Iron Absorption Line from Luminous Accreting Neutron Star SMC X-1
- The XMM Newton and INTEGRAL observations of the supergiant fast X-ray transient IGR J16328-4726
- X-ray outflows of active galactic nuclei warm absorbers: A 900 ks Chandra simulated spectrum