Welcome to tstrippy's documentation =================================== tstrippy is a research code for modeling stellar stream formation, with an initial focus on stars escaping from globular clusters within the Milky Way. It provides gravitational potential models and numerical tools for integrating Hamiltonian equations of motion. This package was developed by yours truly, `Salvatore Ferrone `_, for the simulations presented in my `PhD thesis `_. It is not intended to replace mature community packages such as `galpy `_, `gala `_, or `Agama `_. Instead, it is a focused tool built for a specific scientific problem. If you use this package and have questions, feel free to reach out: salvatore.ferrone.1996@gmail.com. Precomputed predictions for escaped tidal debris from Milky Way globular clusters are available `here `_. Documentation roadmap --------------------- This documentation is organized into three sections: 1. Package basics: loading included data products (currently the globular cluster catalog) and working with the built-in gravitational potential models. 2. Orbit integration in the Galaxy: solving for trajectories of point masses in different Galactic potentials. 3. Stream disruption workflows: simulating stream formation/disruption and validating that the method behaves as expected. .. toctree:: :maxdepth: 1 :caption: Installation installation.rst .. toctree:: :maxdepth: 1 :caption: Package basics baumgardt_catalog.ipynb .. toctree:: :maxdepth: 1 :caption: Orbit integration in the Milky Way galactic_orbits.ipynb reverse_integrability_vanilla.ipynb bar.ipynb reverse_integrability_bar.ipynb .. toctree:: :maxdepth: 1 :caption: Stream disruption examples stream_generation.ipynb bar_stream_example.ipynb