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Manzini Federico Crippa Roberto Oldani Virgino Guaita Cesare 《Earth, Moon, and Planets》1999,87(2):73-85
Using a CCD camera attached to the 0.335 m and 0.20 m reflectors of S.A.S. Observatory (Novara, Italy), we followed the linear
jets and shells of comet Hale–Bopp between May 1996 and May 1997. In addition to confirming the model of Sekanina and Bohenhardt
(1997), the study of the linear jets provided indications concerning the orientation of the comet's axis of rotation over
time. The study of the shells revealed that the speed at which they move away from the nucleus was not constant. A periodic
variation of the shell expansion velocity may not be excluded : if so, a possible precessional effect on the axis of rotation
of the comet's nucleus could explain this behavior.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
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