Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-28T07:38:17.482Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Correlation of the FIR and Radio Radiation of Spiral Galaxies

Published online by Cambridge University Press:  19 July 2016

H. M. Tovmassian
H. M. Tovmassian*
Affiliation:
INAOE, AP 51 y 216, 72000, Puebla, Pue, Mexico

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The comparison of the Byurakan classification of central parts of galaxies with the results of their radio observations showed that there is a definite correlation: the radio emission is more often observed in those galaxies which were suggested to have active nuclei.

Type
Poster Contributions: Continuum studies
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 337
Copyright
Copyright © Kluwer 1994 

References

Sofier, B.T., Sanders, D.B., Madore, B.F., Neugebauer, G., Danielson, G.E., Elias, J.H., Lonsdale, C. & Rice, W.L. 1987. ApJ, 320, 238.Google Scholar
Tovmassian, H.M. 1982. Astrofisika, 18, 25.Google Scholar