Skip to content

A Python function to automatically quantify the dense core alignment based on the 2D spatial distribution of cores.

License

Notifications You must be signed in to change notification settings

Anchewei/ALPara

Folders and files

NameName
Last commit message
Last commit date

Latest commit

 

History

17 Commits
 
 
 
 
 
 
 
 
 
 
 
 
 
 

Repository files navigation

alt text

Alignment Parameters: Quantifying Dense Core Alignment in Star-forming Regions

Alignment parameters utilize 2D core positions and core weights to quantitatively assess core alignment. These parameters offer an objective, automated and reproducible method for measuring core alignment, with higher values indicating more aligned configurations and lower values suggesting more clustered arrangements. To employ these parameters as a two-label classification tool, a threshold of 3.3 can be used to differentiate between "clustered" and "aligned" categories.

alt text

If these alignment parameters are used in published work, please cite the relevant paper. This paper details the derivation of the parameters, their performance testing, and the determination of the classification threshold. Additionally, the parameters are applied to the 1.3 mm dust continuum images from the ASHES survey (PI: P. Sanhueza) to investigate the relationship between core alignment and clump-scale properties.

Dependencies

  • NumPy,
  • Matplotlib

Using the code

An example notebook, TestClump.ipynb, demonstrates how to use the functions to calculate alignment parameters and reproduce the test clumps described in Section 2.1 of the accompanying paper.

About

A Python function to automatically quantify the dense core alignment based on the 2D spatial distribution of cores.

Resources

License

Stars

Watchers

Forks

Packages

No packages published