Abstract
Dent and Haddock1 have investigated the high-frequency part of the NGC 1275 spectrum and found that the flux density increases between 3 and 10 GHz by about a factor of two.
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References
Dent, W. A., and Haddock, F. T. (preceding communication).
Lynds, C. R., and Sobiesky, S., Publ. Nat. Rad. Astro. Obs., 1, 155 (1961).
Leslie, P. R. R., and Elsmore, B., Observatory, 81, 14 (1961).
Heeschen, D. S., and Meredith, B. L., Publ. NRAO, 1, 121 (1961).
Baars, J. W. M., Mezger, P. G., and Wendker, H. (in the press).
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BAARS, J., MEZGER, P. & WENDKER, H. A Radio Investigation of NGC 1265 and NGC 1275. Nature 205, 488–489 (1965). https://doi.org/10.1038/205488a0
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DOI: https://doi.org/10.1038/205488a0
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