Magellanic-type galaxies

Mathematics – Logic

Scientific paper

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Astrodynamics, Body Kinematics, Galactic Structure, Magellanic Clouds, Astronomical Models, Galactic Evolution, Galactic Rotation, Morphology, Spiral Galaxies, Velocity Distribution

Scientific paper

The morphological structure of Magellanic galaxies (Irr I) is investigated and a classification scheme is established. In addition, the kinematics and dynamics of the Large Magellanic Cloud as the nearest and best known example of a Magellanic-type galaxy are examined. The velocity fields of the LMC are interpreted and a mass model of the LMC is examined.

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