Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-12T19:55:56.406Z Has data issue: false hasContentIssue false
  • English
  • Français

Comet Brightness Parameters: Definition, Determination, and Correlations

Published online by Cambridge University Press:  22 February 2018

David D. Meisel  and
Charles S. Morris

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Visual estimates of comet total magnitude have been made for well over one hundred years. In this paper no attempt has been made to review all previous work on comet magnitudes. Instead we prefer to concentrate on developing a conceptual framework upon which previous work can be evaluated. We have tried to unify the approach as much as possible by filling in gaps that occur between previously published accounts. The present work represents an extension and revision of an earlier attempt at understanding comet magnitudes (Meisel, 1970).

Type
Part I
Information
International Astronomical Union Colloquium , Volume 25 , Issue Part1: The Study of Comets , 1976 , pp. 410 - 444
Copyright
Copyright © NASA 1976

References

Beyer, M. 1950, A.N. 278, 217.Google Scholar
Beyer, M. 1952, “La Physique des Comètes”, Mém. Soc. Roy. de Liège 13, 236 Google Scholar
Beyer, M. 1970, A.N. 291, 257.Google Scholar
Beyer, M. 1972, A.N. 293., 241.Google Scholar
Bobrovnikoff, N. T. 1941a, Contrib. Perkins Obs., Nos. 15 and 16.Google Scholar
Bobrovnikoff, N. T. 1941b, Pop. Astron. 49, 478.Google Scholar
Bobrovnikoff, N. T. 1951, Astrophysics, Hynek, J. A., Ed. (McGraw-Hill, New York), Chap. 7.Google Scholar
Bortle, J. E. and Milon, D. 1971, Strolling Astron. 23, 99.Google Scholar
Bortle, J. E. and Milon, D. 1973, ibid., 24, 75.Google Scholar
Delsemme, A. 1973a, Astrophysical Letters J4, 163.Google Scholar
Delsemme, A. 1973b, ibid.Google Scholar
Delsemme, A. 1973c, Sp. Sci. Rev. 15, 89.Google Scholar
Goodman, J. W. 1968, Introduction to Fourier Optics (McGraw-Hill, New York).Google Scholar
Haser, L. 1957, Bull. Acad. Sci. Belgique 43, 740.Google Scholar
Huebner, W. F. 1965, Z. Astrophys. 63, 22.Google Scholar
Levin, B. J. 1943, Sov. AJ 25, 246,Google Scholar
Marsden, B. G. 1972, Qu Journ. R.A.S. 13, 415.Google Scholar
Meisel, D. D. 1970, A. J. 75, 252.Google Scholar
Morris, C. S. 1973a, P.A.S.P. 85, 470.Google Scholar
Morris, C. S. 1973b, Strolling Astronomer, 24, 68.Google Scholar
Morris, C. S. 1974, Strolling Astronomer, 24, 198.Google Scholar
Morris, C. S. and Bortle, J. E. (1973), P.A.S.P. 85, 249.Google Scholar
O'Dell, C. R., and Osterbrock, D. E. 1962, Astrophys. J. 136, 559.Google Scholar
Ooft, J., 1950, Bull. Ast. Inst. Ned. 11, 91.Google Scholar
Oort, J., and Schmidt, M. 1951, Bull. Astron. Inst. Neth. 11, 259.Google Scholar
Öpik, E. J. 1963, Irish Astron. J. 6, 93.Google Scholar
Richter, N. B. 1963, The Nature of Comets (Methuen and Co., London).Google Scholar
Schmidt, M. 1951, Bull. Astron. Inst. Neth. 11, 253.Google Scholar
Sidgwick, J. B. 1955, Observational Astronomy for Amateurs (Faber and Faber, London), p. 251.Google Scholar
Vanýsek, V. 1952, Contrib. Inst. Brno 1, No. 9.Google Scholar