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Cited by
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This article has been cited by the following publications. This list is generated based on data provided by Crossref.
Slee, O. B. Tuohy, I. R. Nelson, G. J. and Rennie, C. J. 1981. Microwave emission from flare star AT Mic. Nature, Vol. 292, Issue. 5820, p. 220.
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  • Google Scholar
Innis, J. L. Coates, D. W. Thompson, K. Nelson, G. J. Slee, O. B. and Wright, Alan E. 1985. An Optlcal and Radio Investigation of the Active RS CVn Star HD 127535. Publications of the Astronomical Society of Australia, Vol. 6, Issue. 2, p. 160.
  • CrossRef
  • Google Scholar
Bunton, John D. Stewart, R. T. Slee, O. B. Nelson, G. J. Wright, Alan E. Corbin, Julian B. Brown, David R. and Hall, P. J. 1986. Radio Emission from Starspots on RSCVn Binary HR1099. Publications of the Astronomical Society of Australia, Vol. 6, Issue. 3, p. 316.
  • CrossRef
  • Google Scholar
Stewart, R. T. Slee, O. B. Nelson, G. J. Wright, Alan E. Jauncey, David L. Large, M. I. Bunton, John D. Vaughan, A. E. and Peters, W. L. 1987. Cool Stars, Stellar Systems, and the Sun. Vol. 291, Issue. , p. 95.
  • CrossRef
  • Google Scholar
Beardwood, R. J. and Melrose, D. B. 1990. Two Models for the Radio Spectra of Stellar Flares. Publications of the Astronomical Society of Australia, Vol. 8, Issue. 3, p. 283.
  • CrossRef
  • Google Scholar
Stewart, R. T. 1992. Eruptive Solar Flares. Vol. 399, Issue. , p. 301.
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Interpretation of a Correlation between the Flux Densities of Extended Hard X-ray and Microwave Solar Bursts
  • Volume 3, Issue 6
  • G. J. Nelson (a1) and R. T. Stewart (a1)
  • DOI: https://doi.org/10.1017/S1323358000026205
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Interpretation of a Correlation between the Flux Densities of Extended Hard X-ray and Microwave Solar Bursts
  • Volume 3, Issue 6
  • G. J. Nelson (a1) and R. T. Stewart (a1)
  • DOI: https://doi.org/10.1017/S1323358000026205
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Interpretation of a Correlation between the Flux Densities of Extended Hard X-ray and Microwave Solar Bursts
  • Volume 3, Issue 6
  • G. J. Nelson (a1) and R. T. Stewart (a1)
  • DOI: https://doi.org/10.1017/S1323358000026205
Available formats Please select a format to save.
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