Active inner regions of isolated galaxies

Details Active inner regions of isolated galaxies Active inner regions of isolated galaxies

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984xue..conf...21d&link_type=abstract

In Max-Planck Inst. für Physik und Astrophysik X-Ray and UV Emission from Active Galactic Nuclei p 21-24 (SEE N85-17790 08-88)

Astronomy and Astrophysics

Astrophysics

1

Galactic Nuclei, Stellar Evolution, Ultraviolet Radiation, Astronomical Models, Astronomical Spectroscopy, Mass Distribution, Spectral Energy Distribution

Scientific paper

Very isolated galaxies were observed in spectral regions from 5 GHz to 2500 THz. Nuclear UV excesses are found to be a general phenomenon. This is interpreted as indicating that in isolated galaxies the inner regions are more active in forming stars than in nonisolated galaxies. The occurrence of star formation deeper in the gravitational well may be the reflection of a real difference in mass distribution between isolated and nonisolated objects.

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