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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

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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