tests:collision:gc3
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GC III
Goals/projects for GC III workshop
A. Method comparison (now Challenge #4):
Jeans modelling vs. Distribution-function based models for fitting mock data of GCs. We will start with $N$-body snapshots of the M4 models by Heggie (2014): http://datashare.is.ed.ac.uk/handle/10283/618
B. Understanding Gaia errors:
What will Gaia actually give us (for GCs, open clusters, runaway stars, hypervelocity stars)? What can we do with TGAS?
C. Potential escapers:
a) quantify biases from ignoring them
b) towards self-consistent mixture models with potential escapers
D. Rotation:
include prescription for rotation in multi-mass DF models.
tests/collision/gc3.1441104144.txt.gz · Last modified: 2022/10/24 12:26 (external edit)