Figure 4 from Gas Jet Morphology and the Very Rapidly Increasing Rotation Period of Comet 41P/Tuttle–Giacobini

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Gas Jet Morphology and the Very Rapidly Increasing Rotation Period of Comet 41P/Tuttle–Giacobini–Kresák

Authors: David G. Schleicher, Matthew M. Knight, Nora Eisner, and Audrey Thirouin

2019 The Astronomical Journal 157 108.

Provider: AAS Journals

Caption: Figure 4.

Sample CN image pairs used to derive the apparent period. In each case shown, the matching images must be a whole number of rotational cycles apart. Scaling is the same as in previous figures.

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