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Titlebook: Cometary Science after Hale-Bopp; Volume 2 Proceedings H. Boehnhardt,M. Combi,R. Schulz Conference proceedings 2002 Springer Science+Busine

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https://doi.org/10.1007/978-94-011-4028-7 one orbit revolution after the splitting of its nucleus in 1995 (Boehnhardt et al., 1995). Fragment C was found back with coma in November 1999 at 4 AU inbound and it continued to be active during the perihelion arc until at least December 2001 when we observed it last at 3.3 AU outbound. Fragment
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Address to the World Bank Sociological GroupRAS (Northern Caucuses, Nizhny Arkhyz) on July 23/24, 26/27 and 27/28, 2000. On July 22/23, before the splitting of the cometary nucleus, several emission lines, such as C., C., CN, NH, CH, NH., CO., H.O. were clearly identified in the spectra. The inspections of the CCD spectra obtained on July 27/
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Address to the World Bank Sociological Group6). In this paper we report the first results of our extensive imaging and spectroscopic monitoring campaign with ESO telescopes over several weeks before and after the perihelion passage on May 25 2001.
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Social Analysis in the World Bank2 (LINEAR), which can be related to the group of split comets. Comets West, S4 (LINEAR) and A2 (LINEAR) were observed during splitting. We compare the polarimetric measurements of the dust particles in these comets, sometimes together with available photometric and colorimetric data, with those in n
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Split Comet C/2001 A2 (LINEAR)6). In this paper we report the first results of our extensive imaging and spectroscopic monitoring campaign with ESO telescopes over several weeks before and after the perihelion passage on May 25 2001.
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