Abstract
Frank Kerr and I first met in 1952, when he was on the staff of the CSIRO Radiophysics Division, then housed on the grounds of the University of Sydney, and I was working at Mount Stromlo Observatory as the first Research Fellow of the newly created Astronomy Department of the Australian National University in Canberra.
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References
Kerr, F. J. 1941, Refractive Indexes of Gases at High Radio Frequencies, Nature 148, 751, 752.
Kerr, F. J. 1943, Refractive Indices of Gases at High Radio Frequencies, Proc. Phys. Soc. 55, 92–98.
Kerr, F. J. 1948, Radio Superrefraction in the Coastal Regions of Australia, Australian J. Sci. Res. Al, 443–463.
Kerr, F. J., Shain, C. A., and Higgins, C. S. 1949, Moon Echoes and Penetration of the Ionosphere, Nature 163, 310–313.
Ewen, H. I. and Purcell, E. M.1951, Radiation from Galactic Hydrogen at 1420 Mc/s, Nature 168
Muller, C. A. and Oort, J. H. 1951, The Interstellar Hydrogen Line at 1420 Mc/s and an Estimate of Galactic Rotation, Nature 168, 357–358.
(Christiansen, W. N. and Hindman, J. V. 1951), (Announcement of Detection of the 21 cm Hydrogen Line), Nature 168, 358.
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Kerr, F. J. 1952, On the Possibility of Obtaining Radar Echoes from the Sun and Planets, Proc. IRE 40, 660–666.
Kerr, F. J., Hindman, J. V., and Robinson, B. J. 1954, Observations of the 21-cm Line from the Magellanic Clouds, Australian J. Phys. 7, 297–314.
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Kerr, F. J. and de Vaucouleurs, G. 1956, The Masses of the Magellanic Clouds from Radio Observations, Australian J. Phys. 9, 90–111.
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Oort, J. H., Kerr, F. J., and Westerhout, G. 1958, The Galactic System as a Spiral Nebula, Mon. Not. Roy. Astron. Soc. 118, 379–389.
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Kerr, F. J. 1962a, Galactic Velocity Models and the Interpretation of 21-cm Surveys, Mon. Not. Roy. Astron. Soc. 123, 327–345.
Kerr, F. J. 1962b, 210-foot Radio Telescope's First Results, Sky and Tel. 24, 254–260.
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McKechnie, M.; Kerr, F. J., and Hill, E. R. 1963, Radio Astronomy Bibliography, 1957–1960, Radiophysics Lab Report RPL 168 (309 pp.).
Kerr, F. J. and Rodgers, A. W. (eds.) 1964, The Galaxy and the Magellanic Clouds, Proc. of IAU Symp. No. 20 (March 1963) (Canberra: Australian Academy of Science).
Kerr, F. J. and Westerhout, G. 1965, Distribution of Hydrogen in the Galaxy, pp. 167–202 in Galactic Structure (eds. A. Blaauw and M. Schmidt), Vol. 5 of Stars and Stellar Systems (Chicago: Univ. of Chicago Press).
Kerr, F. J 1968., Radio-line Emission and Absorption by the Interstellar Gas, pp. 575–622 in Nebulae and Interstellar Matter (eds. B. M. Middlehurst and L. H. Aller), Vol. 7 of Stars and Stellar Systems (Chicago: Univ. of Chicago Press).
Kerr, F. J. and Simonson, S. C., III (eds.) 1974, Galactic Radio Astronomy, Proc. of IAU Symp. No. 60 (September 1973) (Dordrecht: Reidel).
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de Vaucouleurs, G. (1988). Some reminiscences of frank kerr and the work on the milky way and the magellanic clouds. In: Blitz, L., Lockman, F.J. (eds) The Outer Galaxy. Lecture Notes in Physics, vol 306. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-19484-3_39
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DOI: https://doi.org/10.1007/3-540-19484-3_39
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