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JWST and Gemini Observations of the Active Centaur 450P/LONEOS: Nucleus and Coma Characterizations

  • Authors: Charles A. Schambeau, Michael S. P. Kelley, Maria Womack, Eva Lilly, Theodore Kareta, Sara Faggi, Olga Harrington Pinto, Marco Micheli, Dominique Bockelée-Morvan, Yanga R. Fernández, Adam McKay, Noemi Pinilla-Alonso, Javier Licandro, Aren Beck, Geronimo L. Villanueva, James Bauer, Lori Feaga, Michael A. DiSanti, Kacper Wierzchos

Charles A. Schambeau et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 3.

Normalized radial surface brightness profiles of the Gemini-N 450P images on 2022 August 21 (r﹩{}^{{\prime} }﹩; left panel) and 2022 September 27 (g﹩{}^{{\prime} }﹩; right panel). Surrounding field star profiles are overplotted with a gray shaded region representing their range of scatter. 450P’s profiles are similar to those of the field stars, which is consistent with little to no dust coma present.

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