Self-consistent Modelling of the Milky Way using Gaia data
classification
🌌 astro-ph.GA
keywords
datadistributionfunctiongaiamilkyaccuracyactionangle
read the original abstract
Angle/action based distribution function (DF) models can be optimised based on how well they reproduce observations thus revealing the current matter distribution in the Milky Way. Gaia data combined with data from other surveys, e.g. the RAVE/TGAS sample, and its full selection function will greatly improve their accuracy.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.