Accretion disk dynamics, photoionized plasmas, and stellar opacities

Details Accretion disk dynamics, photoionized plasmas, and stellar opacities Accretion disk dynamics, photoionized plasmas, and stellar opacities

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009phpl...16d1001m&link_type=abstract

Physics of Plasmas, Volume 16, Issue 4, pp. 041001-041001-11 (2009).

Physics

8

Accretion And Accretion Disks, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Mhd Waves, Plasma Waves, Turbulence, Magnetohydrodynamics And Plasmas, Magnetohydrodynamic And Fluid Equation, Magnetohydrodynamics

Scientific paper

We present a brief review on the atomic kinetics, modeling and interpretation of astrophysical observations, and laboratory astrophysics experiments. The emphasis is on benchmarking of opacity calculations relevant for solar structure models, photoionized plasmas research, the magnetohydrodynamic numerical simulation of accretion disk dynamics, and a connection between radiation transport effects and plasma source geometry details. Specific cases of application are discussed with relevance to recent and proposed laboratory astrophysics experiments as well as Chandra and X-ray Multi-Mirror Mission Newton observations.

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