https://github.com/m-wells/eclipsingbinarystars.jl

Provides an eclipsing binary type as well as functions that compute eclipsing binary parameters
https://github.com/m-wells/eclipsingbinarystars.jl

Last synced: 3 months ago
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Provides an eclipsing binary type as well as functions that compute eclipsing binary parameters

• Host: GitHub
• URL: https://github.com/m-wells/eclipsingbinarystars.jl
• Owner: m-wells
• License: agpl-3.0
• Created: 2018-07-23T14:43:46.000Z (almost 7 years ago)
• Default Branch: master
• Last Pushed: 2024-02-25T20:09:56.000Z (over 1 year ago)
• Last Synced: 2025-01-20T17:55:04.413Z (5 months ago)
• Language: Jupyter Notebook
• Homepage:
• Size: 385 KB
• Stars: 2
• Watchers: 2
• Forks: 0
• Open Issues: 6
• Metadata Files:
  • Readme: README.md
  • License: LICENSE

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README

        
# EclipsingBinaryStars.jl

[![Build Status](https://travis-ci.com/m-wells/EclipsingBinaryStars.jl.svg?token=qtRCxXQJn8B2HN1f6h3k&branch=master)](https://travis-ci.com/m-wells/EclipsingBinaryStars.jl)

Provides methods for doing simple analysis of detached binary stars

* Determine (if any) the eclipse morphology of a system

* If the system eclipses, determine the eclipse duration

* determine if the system is experiencing Roche Lomb overflow

* get a spherical star approximation of the transit flux depth (no limb darkening yet)