activity
20142019
most citedEvolution of CO, CH, and OCS abundances relative to HO in the coma of comet 67P around perihelion from Rosetta/VIRTIS-H observations

88 citations · 405 across the 7 of their papers we have counts for

collaborators

6 papers

astro-ph.EP201961 cited

Pluto's Haze as a Surface Material

W. M. Grundy, T. Bertrand, R. P. Binzel +37

Pluto's atmospheric haze settles out rapidly compared with geological timescales. It needs to be accounted for as a surface material, distinct from Pluto's icy bedrock and from the…

astro-ph.EP201960 cited

Formation of Charon's Red Poles From Seasonally Cold-Trapped Volatiles

W. M. Grundy, D. P. Cruikshank, G. R. Gladstone +38

A unique feature of Pluto's large satellite Charon is its dark red northern polar cap. Similar colours on Pluto's surface have been attributed to organic macromolecules produced by…

astro-ph.EP201947 cited

The CH4 cycles on Pluto over seasonal and astronomical timescales

T. Bertrand, F. Forget, O. M. Umurhan +13

New Horizons observations suggest that CH4 on Pluto has a complex history, involving reservoirs of different composition, thickness and stability controlled by volatile processes o…

astro-ph.EP201688 cited

Evolution of CO, CH, and OCS abundances relative to HO in the coma of comet 67P around perihelion from Rosetta/VIRTIS-H observations

D. Bockelée-Morvan, J. Crovisier, S. Erard +19

Infrared observations of the coma of 67P/Churyumov-Gerasimenko were carried out from July to September 2015, i.e., around perihelion (13 August 2015), with the high-resolution chan…

astro-ph.EP201645 cited

Detection of exposed HO ice on the nucleus of comet 67P/Churyumov-Gerasimenko

M. A. Barucci, G. Filacchione, S. Fornasier +42

Since the orbital insertion of the Rosetta spacecraft, comet 67P/Churyumov-Gerasimenko (67P/C-G) has been mapped by OSIRIS camera and VIRTIS spectro-imager, producing a huge quanti…

astro-ph.EP201444 cited

How to link the relative abundances of gas species in coma of comets to their initial chemical composition ?

Ulysse Marboeuf, Bernard Schmitt

The chemical composition of comets is frequently assumed to be directly provided by the observations of the abundances of volatile molecules in the coma. The present work aims to d…