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Probabilistic distribution functions
DOI:10.1093/mnras/stab2047.png)
Abstract
En 中文
Observed clusters should be modelled by considering the distribution function (DF) to be a random variable that quantifies the degree of excitation of the system's normal modes. A system of canonical coordinates for the space of DFs are identified so DFs can be weighted in a consistent way.
Keywords:
methods: analytical
Galaxy: kinematics and dynamics
galaxies: kinematics and dynamics
Journal
IF:
4.8
Papers:
7.0W
Citations:
25.0W

