Emission band and continuum photometry of Comet West (1975n) - I. Heliocentric dependence of the flux in the emission bands and the continuum
Open Access
- 1 December 1979
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 189 (4) , 897-906
- https://doi.org/10.1093/mnras/189.4.897
Abstract
Spectrum scans of the coma of Comet West (1975n) covering the range $$\lambda \lambda \,3700-5700$$ Å were made on eight nights when the heliocentric distance of the comet varied from 0.588 to 0.853 AU. These have been used to derive the absolute flux in the CN (0, 0), C3 (4050), C2 (1, 0) and C2 (0, 0) bands as well as in the continuum. Enhancements in the band emissions were noticed on three nights in CN (0, 0), C3 (4050) and C2 (1, 0). The column densities of neutral sodium atoms are derived from scans around 5900 A on four nights. The column densities of CO+ ions corresponding to four prominent band sequences are evaluated from two scans of the tail.
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