2017
DOI: 10.1017/s1743921317007049 View full text |Buy / Rent full text
|
|

Abstract: Galaxy models are fundamental to exploiting surveys of our Galaxy. There is now a significant body of work on axisymmetric models. A model can be defined by giving the DF of each major class of stars and of dark matter. Then the self-consistent gravitational potential is determined. Other modelling techniques are briefly considered before an overview of some early work on non-axisymmetric models.

Help me understand this page
View preprint versions

Search citation statements

Order By: Relevance
0
0
0
0
0
0
4
0

Publication Types

Select...

Relationship

0
0

Authors

Journals