Abstract
Spectrophotometric observations of Cornet Hartley-Good (19851) during five nights in 1985 are presented in the wavelength range λλ3200–7000 ». The emission bands due to CN, CH, C2, and C3 molecules are observed. The abundances (N) and production rates (Q) of the molecules are derived.
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Rautela, B.S., Goraya, P.S., Sanwal, B.B. et al. Spectrophotometric observations of comet Hartley-Good (1985l). Earth Moon Planet 40, 21–27 (1988). https://doi.org/10.1007/BF00057944
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DOI: https://doi.org/10.1007/BF00057944