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Stellar Bow Shocks.pdf

1005.1527.pdf
Preview of Stellar Bow Shocks
🔗 Source: arxiv.org
📊 Size: 973 KB
👤 Author: amelia
⬇️ Downloads: 128

Summary

Stellar bow shocks occur when a star's stellar wind collides with the interstellar medium, creating a shock wave. The shock wave is the boundary between the stellar wind and the interstellar medium, and is characterized by a dramatic change in density and pressure. Observations of stellar bow shocks can be enhanced using image processing techniques, such as the AstroFracTool software, which can reveal details such as edges and faint objects. The physics of shock waves is based on fluid mechanics modeling, and can be described by the Rankine-Hugoniot equations, which relate the density, pressure, and flux conditions on either side of the shock. Shock waves can occur in various astrophysical contexts, including the interaction between the solar wind and the interstellar medium, and can be studied using observations from space telescopes such as Spitzer and Akari.

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Description

Stellar bow shocks occur when a star's stellar wind collides with the interstellar medium, creating a shock wave.

Technical Information

  • File Format: PDF
  • File Size: 973 KB
  • Pages: 9
  • Language: EN
  • Author: amelia
  • Total Downloads: 128
  • Last Updated: 1 week ago

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