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A Radio Investigation of NGC 1265 and NGC 1275

Nature volume 205, pages 488–489 (1965)Cite this article

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

  1. Dent, W. A., and Haddock, F. T. (preceding communication).

  2. Lynds, C. R., and Sobiesky, S., Publ. Nat. Rad. Astro. Obs., 1, 155 (1961).

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  3. Leslie, P. R. R., and Elsmore, B., Observatory, 81, 14 (1961).

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  4. Heeschen, D. S., and Meredith, B. L., Publ. NRAO, 1, 121 (1961).

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  5. Baars, J. W. M., Mezger, P. G., and Wendker, H. (in the press).

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Authors and Affiliations

  1. National Radio Astronomy Observatory (Operated by Associated Universities, Inc., under contract with the U.S. National Science Foundation), Green Bank, West Virginia

    J. W. M. BAARS, P. G. MEZGER & H. WENDKER

Authors
  1. J. W. M. BAARS
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  2. P. G. MEZGER
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  3. H. WENDKER
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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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