The statistics of structure and rotation of disk galaxies

Details The statistics of structure and rotation of disk galaxies The statistics of structure and rotation of disk galaxies

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980acasn..21..200h&link_type=abstract

Acta Astronomica Sinica, vol. 21, June 1980, p. 200-207. In Chinese, with abstract in English.

Mathematics

Logic

Disk Galaxies, Galactic Evolution, Galactic Rotation, Galactic Structure, Celestial Mechanics, Hubble Diagram, Light Curve, Mass Ratios, Radio Emission, Statistical Analysis

Scientific paper

The optical and radio rotation curves of 57 galaxies are analyzed. The dynamical characteristics of structure and rotation of disk galaxies are found to vary systematically from early type to later type along the Hubble sequence. The dispersions of the dynamical characteristics in each morphological type are related to galaxy mass, and the dynamic state of the galaxies is also affected by tidal action.

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