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Studying the longterm evolution of gas activity in the coma of Comet C/1995 O1 (Hale-Bopp), with a special focus on the chemistry of carbon bearing molecules
[article]
2003
The starting point for this work was the dataset obtained during the optical longtermmonitoring program of comet C/1995 O1 Hale-Bopp [Rauer et al., 1997, 2002]. Observations started in April 1996 and ended nearly 5 years later in January 2001 covering a heliocentric distance range from 4.6-2.8 AU pre- perihelion and from 2.9-12.8 AU post-perihelion. It was the longest campaign ever observing a single comet in the optical wavelengths range so far. This huge dataset had to be reduced and
doi:10.17169/refubium-11390
fatcat:qzvxv7wvanfgpgehhwprwolqbm