John Edward Dyson
Affiliations: | 1966 | University of Manchester, Manchester, England, United Kingdom |
Website:
https://academic.oup.com/astrogeo/article/51/4/4.40/197337Google:
"John Dyson"Mean distance: (not calculated yet)
Children
Sign in to add traineeTom P. Ray | grad student | 1981 | University of Manchester (Astronomy Tree) |
William J. Henney | grad student | 1989-1992 | The University of Manchester (Astronomy Tree) |
S. Jane Arthur | post-doc | 1991-1992 | University of Manchester |
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Publications
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Dyson JE, Williams RJR, Perry JJ. (1996) Line Forming Regions in Active Galaxies and Their Nuclei Astrophysics and Space Science. 237: 187-206 |
Hartquist TW, Dyson JE, Williams RJR. (1996) Wide intermediate scale structures in mass-loaded flows Astrophysics and Space Science. 235: 165-168 |
Dyson JE, Williams RJR, Redman MP. (1995) Clumpy Ultra Compact HII Regions - Part One - Fully Supersonic Wind-Blown Models Monthly Notices of the Royal Astronomical Society. 277: 700-704 |
Hartquist TW, Durisen RH, Dyson JE, et al. (1995) Can dust formation in evolved stars be suppressed near active galactic nuclei? Astrophysical Journal. 453: 77-82 |
Williams RJR, Hartquist TW, Dyson JE. (1995) The Weakening of the Termination Shocks of Isothermal Winds by Mass Loading The Astrophysical Journal. 446: 759 |
Redman MP, Williams RJR, Dyson JE. (1995) All's knot quiet on the recombination front Astrophysics and Space Science. 233: 195-198 |
Dyson JE, Williams RJR, Perry JJ. (1995) Flows and Shocks in Active Galaxies and their Nuclei Astrophysics and Space Science. 233: 199-214 |
Arthur SJ, Dyson JE, Hartquist TW. (1994) Mass-loaded flows – VII. Transonic flows from the cores of planetary nebulae Monthly Notices of the Royal Astronomical Society. 269: 1117-1122 |
Dyson JE, Hartquist TW. (1994) Mass-loaded flows - VI. A tale of the Galactic Centre Monthly Notices of the Royal Astronomical Society. 269: 447-450 |
Meaburn J, Dyson JE, Goudis CD, et al. (1994) An Evolutionary Model For the Wolf Rayet Nebula NGC 2539 Astrophysics and Space Science. 216: 281-283 |