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3.18. Observational data implying the NGC 1275 nucleus complexity

Published online by Cambridge University Press:  25 May 2016

I. Pronik
I. Pronik*
Affiliation:
Crimean Astrophysical Observatory, 334413, p/o Nauchny, Crimea, Ukraine

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The central unresolved source of the galaxy NGC 1275 in red has a dimension of about 8″, but in blue its bright part is about of 0.″5. HST observations, obtained with the filter λ 2200Å cannot reveal the structure of the source inside 0.″26. Now we have collected the observed features of NGC 1275 nucleus in optics and radio domains, which are possibly associated with the complex structure of the nucleus.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 125 - 126
Copyright
Copyright © Kluwer 1998 

References

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Pronik, V.I., 1987. In Proc. IAU Sym 121, eds. Khachikian, E. et al., 191.Google Scholar