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README <<<<<<< HEAD

Thesis

This is my PhD thesis called: "Estudio de la Interacción de Flujos Múltiples de Fuentes Astrofísicas Aplicada a los Proplyds Clásicos de la Nebulosa de Orión"

Chapter 1: Orion Nebula

- General Characteristics
- Proplyds

Chapter 2: Bow Shocks

- Proplyds
- LL Objects
- Runaway Stars
- AGB and Supergiant Stars

Chapter 3: Fundamental Concepts

- Fundamental Parameters
- Planitude and Alatude
- Quadrics of Revolution
- Projection Onto the Plane of Sky

Chapter 4: Thin Shell Model

- Introduction
- Conserved Quantities
- Two Winds interaction Problem
- True Shape of obtained Bow Shocks
- Apparent Shape

Chapter 5: Results Obtained for Classical Proplyds

- Methodology
- Comparison With Thin Shell Model
- Obtention of Stagnation Pressure

Chapter 6: Summary and Conclusions

Appendix

 - HII Regions
 - Shocks and Ionization Fronts
 - Rotation Matrix
 - Mathematical Derivation of Radius of Curvature
 - Step by Step Derivation of Characteristic Radii
 - True Versus Apparent Shapes of Bow Shocks

======= bowshock-shape

Calculate shape of wind-wind bowshocks

Python scripts written by Jorge to calculate the shape of an axisymmetric bowshock due to the interaction between a proplyd flow and a stellar wind.

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