CO and Other Volatiles in Distantly Active Comets

@article{Womack2017COAO,
  title={CO and Other Volatiles in Distantly Active Comets},
  author={Maria Womack and Gal Sarid and Kacper Wierzchos University of South Florida and Florida Space Institute and University of Central Florida},
  journal={Publications of the Astronomical Society of the Pacific},
  year={2017},
  volume={129},
  pages={031001}
}
  • M. Womack, G. Sarid, U. Florida
  • Published 31 October 2016
  • Physics, Geology
  • Publications of the Astronomical Society of the Pacific
Activity of most comets near the Sun is dominated by sublimation of frozen water, the most abundant ice in comets. Some comets, however, are active well beyond the water-ice sublimation limit of ~3 AU. Three bodies dominate the observational record and modeling efforts for distantly active comets: the long-period comet C/1995 O1 Hale-Bopp and the short-period comets (with Centaur orbits) 29P/Schwassmann Wachmann 1 and 2060 Chiron. We summarize what is known about these three objects emphasizing… 

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