The rapid stellar rotation of radio galaxies

Details The rapid stellar rotation of radio galaxies The rapid stellar rotation of radio galaxies

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207..361j&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, March 15, 1984, p. 361-367.

Astronomy and Astrophysics

Astronomy

7

Angular Velocity, Elliptical Galaxies, Radio Galaxies, Stellar Rotation, Astrodynamics, Galactic Nuclei, Stellar Magnitude, Velocity Distribution, Visible Spectrum

Scientific paper

It is shown from the kinematical data available that radio-emitting
elliptical galaxies tend to rotate more quickly than their radio-quiet
peers. Processes occurring on nuclear scales (a parsec or less) are thus
linked to the large-scale properties of the galaxies.

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