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A model of our Galaxy

Published online by Cambridge University Press:  04 August 2017

U. Haud ,
M. Jôeveer  and
J. Einasto
U. Haud
Affiliation:
Tartu Astrophysical Observatory
M. Jôeveer
Affiliation:
Tartu Astrophysical Observatory
J. Einasto
Affiliation:
Tartu Astrophysical Observatory

Extract

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The construction of models is the most effective tool for a synthesis of various observational data and for a quantitative study of physical and dynamical structure and evolution of stellar systems. Classical models of spiral galaxies were based on rotational velocities, which were identified with circular velocities. They were designed to represent the galactic attraction force in the radial direction.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 85 - 94
Copyright
Copyright © Reidel 1985 

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