Hydrodynamic and Spectral Simulations of HMXB Winds(Chapter 8. White Dwarf and Neutron Star Isolated and/or Binaries, The Extreme Universe in the Suzaku Era)

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概要

• 論文の詳細を見る

• We describe preliminary results of a global model of the radiatively-driven photoionized wind and accretion flow of the high-mass X-ray binary Vela X-1. The full model combines FLASH hydrodynamic calculations, XSTAR photoionization calculations, HULLAC atomic data, and Monte Carlo radiation transport. We present maps of the density, temperature, velocity, and ionization parameter from a FLASH two-dimensional time-dependent simulation of Vela X-1, as well as maps of the emissivity distributions of the X-ray emission lines.

• 2007-12-19

著者

• Akiyama Shizuka

  Lawrence Livermore National Laboratory

• MAUCHE Christopher

  Lawrence Livermore National Laboratory

• LIEDAHL Duane

  Lawrence Livermore National Laboratory

• PLEWA Tomek

  University of Chicago

関連論文

• Hydrodynamic and Spectral Simulations of HMXB Winds(Chapter 8. White Dwarf and Neutron Star Isolated and/or Binaries, The Extreme Universe in the Suzaku Era)

スポンサーリンク