Skip to content

Navigation Menu

Sign in
Appearance settings

Search code, repositories, users, issues, pull requests...

Provide feedback

We read every piece of feedback, and take your input very seriously.

Saved searches

Use saved searches to filter your results more quickly

Sign up
Appearance settings

olozhika/CARPP

Folders and files

NameName
Last commit message
Last commit date

Latest commit

History

15 Commits

Repository files navigation

CARPP: Core Analysis via Radiative Transfer and Profile Parameters

CARPP is a powerful tool for analyzing dense molecular cores using multi-wavelength dust continuum observations. It leverages 3D radiative transfer under spherical symmetry to derive density, temperature profiles, and spectral index, enabling researchers to distinguish between hydrostatic equilibrium (Bonnor-Ebert spheres) and dynamically collapsing cores (power-law profiles).


🌟 Features

  • 3D Radiative Transfer Modeling: Accurately accounts for temperature gradients and optical depth effects.
  • Multi-Wavelength Data Fitting: Optimizes density and temperature profiles using dust continuum images at different wavelengths.
  • Flexible Profile Models:
    • Generalized Plummer-like density profiles (supports Bonnor-Ebert spheres and power-law regimes).
    • Continuous temperature profiles with customizable central and ambient parameters.
  • Robust Performance: Achieves <10% average parameter error under optimal noise/resolution conditions.

πŸ“₯ Installation and Usage

The CARPP package in this repo is the IDL version of CARPP. To use CARPP, you should:

  1. Download the repo
  2. Make sure you have IDL installed on your device
  3. Add the path of CARPP to your IDL at Preferences - IDL - Paths
  4. Do idl run_carpp.pro in Test_Data folder, it should start to calculate the test core
  5. You may now edit and run run_carpp_template.pro

πŸ“œ Citation

TBC

About

CARPP: Core Analysis via Radiative transfer and Profile Parameters! A 3D radiative transfer molecular core analyzing tool through multi-wavelength dust continuum data. It retrieves density profile and helps distinguishing hydrostatic equilibrium (Bonnor-Ebert spheres) from collapsing cores (power-law regimes).

Topics

Resources

License

Stars

Watchers

Forks

Releases

No releases published

Packages

Contributors

Languages

AltStyle γ«γ‚ˆγ£γ¦ε€‰ζ›γ•γ‚ŒγŸγƒšγƒΌγ‚Έ (->γ‚ͺγƒͺγ‚ΈγƒŠγƒ«) /