Copyright Ian Czekala and collaborators 2014-20
email: [email protected]
This package derives dynamical masses for T Tauri stars using the Keplerian motion of their circumstellar disks, applied to radio interferometric data from the Atacama Large Millimeter Array (ALMA) and the Submillimeter Array (SMA). If you use this code or a derivative of it in your research, we would really appreciate it if you cited the first paper in our series, Czekala et al. 2015 ApJ, 806 154C.
For more information, see the Documentation.