ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

[ascl:1711.016] Thindisk: Protoplanetary disk model

Thindisk computes the line emission from a geometrically thin protoplanetary disk. It creates a datacube in FITS format that can be processed with a data reduction package (such as GILDAS, ascl:1305.010) to produce synthetic images and visibilities. These synthetic data can be compared with observations to determine the properties (e.g. central mass or inclination) of an observed disk. The disk is assumed to be in Keplerian rotation at a radius lower than the centrifugal radius (which can be set to a large value, for a purely Keplerian disk), and in infall with rotation beyond the centrifugal radius.

Code site:
https://github.com/smaret/thindisk
Appears in:
http://adsabs.harvard.edu/abs/2016Natur.538..483T http://adsabs.harvard.edu/abs/2016Natur.535..258C
Bibcode:
2017ascl.soft11016M
Preferred citation method:

http://doi.org/10.5281/zenodo.13823


ascl:1711.016
Add this shield to your page
Copy the above HTML to add this shield to your code's website.
Views: 321