Published March 15, 1984
| Version v1
Journal article
The rapid stellar rotation of radio galaxies
Description
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. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 207
- Journal Issue
- 2
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 361-367
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 15054635
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- DISTRIBUTION; GALAXY NUCLEI; LUMINOSITY; RADIO GALAXIES; ROTATION; STARS; VELOCITY
- Descriptors DEC
- COSMIC RADIO SOURCES; GALAXIES; OPTICAL PROPERTIES; PHYSICAL PROPERTIES