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Neptune's carbon monoxide profile and phosphine upper limits from Herschel/SPIRE: Implications for interior structure and formation

Irwin, P. G. J.; Teanby, N. A.; Moses, J. I.

On Neptune, carbon monoxide and phosphine are disequilibrium species, and their abundance profiles can provide insights into interior processes and the external space environment. Here we use Herschel/SPIRE (Spectral and Photometric Imaging REceiver) observations from 14.9-51.5 cm^-1 to obtain abundances from multiple CO and PH₃

Haumea's thermal emission revisited in the light of the occultation results

Fornasier, S.; Lellouch, E.; Marton, G. +9 more

A recent multi-chord occultation measurement of the dwarf planet (136108) Haumea (Ortiz et al., 2017) revealed an elongated shape with the longest axis comparable to Pluto's mean diameter. The chords also indicate a ring around Haumea's equatorial plane, where its largest moon, Hi'iaka, is also located. The Haumea occultation size estimate (size o…

Corrigendum to "Neptune's carbon monoxide profile and phosphine upper limits from Herschel/SPIRE" (Icarus, vol 319, p86-98, 2019)

Irwin, P. G. J.; Teanby, N. A.; Moses, J. I.

The authors would like to publish the below information which was incorrectly published in its original version.