On the origin of molecular oxygen in cometary comae

K. L. Heritier (), K. Altwegg, J.-J. Berthelier, A. Beth, C. M. Carr, J. Keyser, A. I. Eriksson, S. A. Fuselier, M. Galand, T. I. Gombosi, P. Henri, F. L. Johansson, H. Nilsson, M. Rubin, C. Simon Wedlund, M. G. G. T. Taylor and E Vigren
Additional contact information
K. L. Heritier: Imperial College London
K. Altwegg: University of Bern
J.-J. Berthelier: LATMOS/IPSL-CNRS-UPMC-UVSQ
A. Beth: Imperial College London
C. M. Carr: Imperial College London
J. Keyser: Royal Belgian Institute for Space Aeronomy
A. I. Eriksson: Ångström Laboratory
S. A. Fuselier: Southwest Research Institute
M. Galand: Imperial College London
T. I. Gombosi: University of Michigan
P. Henri: CNRS
F. L. Johansson: Ångström Laboratory
H. Nilsson: Swedish Institute of Space Physics
M. Rubin: University of Bern
C. Simon Wedlund: University of Oslo
M. G. G. T. Taylor: European Space Agency
E Vigren: LATMOS/IPSL-CNRS-UPMC-UVSQ

Nature Communications, 2018, vol. 9, issue 1, 1-4

Date: 2018
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DOI: 10.1038/s41467-018-04972-5

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