Spectrophotometric observations of comet P/Crommelin (1983n)

Details Spectrophotometric observations of comet P/Crommelin (1983n) Spectrophotometric observations of comet P/Crommelin (1983n)

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...144l...5f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 144, no. 1, March 1985, p. L5-L8.

Astronomy and Astrophysics

Astrophysics

4

Comets, Gas Evolution, Spectrophotometry, Abundance, Emission Spectra, Molecular Spectra

Scientific paper

Observations of comet P/Crommelin were conducted from February 28 till April 4, 1984 and permitted the evaluation of the gas production rates of the main gaseous species emitting in the optical window over a five week period. The mean variation of the gaseous output of the comet with the heliocentric distance (post perihelion branch of the orbit) varied approximately as r-4.5, a value often found in comets having accomplished a large number of revolutions around the sun.

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