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Cometary Observations and Variations in Cometary Brightness

Published online by Cambridge University Press:  14 August 2015

S. K. Vsekhsvyatskij
S. K. Vsekhsvyatskij*
Affiliation:
Astronomical Observatory, Kiev University, Kiev, U.S.S.R.

Abstract

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The cometary observation service is surveyed. Absolute magnitudes and other physical characteristics are given for the comets that appeared during 1965–1970. The general laws of cometary brightness, in particular the secular decrease in brightness, are discussed. Remarks are made about the standardization of cometary photometry.

Information

Type
Part I/Observations and Ephemerides
Information
Symposium - International Astronomical Union , Volume 45: The Motion, Evolution of Orbits and Origin of Comets , 1972, pp. 9 - 15
Copyright
Copyright © Reidel 1972 

References

Vsekhsvyatskij, S. K.: 1958, Fizicheskie Kharakteristiki Komet , Moscow. (English translation: 1964, Physical Characteristics of Comets, Jerusalem.) Google Scholar
Vsekhsvyatskij, S. K.: 1966a, Komety 1954–1960 , Moscow.Google Scholar
Vsekhsvyatskij, S. K.: 1966b, Mem. Soc. Roy. Sci. Liège Ser. 5 12, 57.Google Scholar
Vsekhsvyatskij, S. K.: 1967, Komety 1961–1965 , Moscow.Google Scholar
Vsekhsvyatskij, S. K. and Il'ichishina, N. I.: 1970, Komety 1965–1969 (in press).Google Scholar