The hypothesis that water snow controls the vaporization of the nucleus of some comets seems verified from the general order of magnitude of the size of their nucleus and of their nuclear albedo; the largest observed production rates are H and OH which both seem to originate from the photodissociation of H2O, as also confirmed by the scale length of the invisible parent molecule producing OH. However, comet Encke is not uniformly covered by water snow, as it produces only one tenth of the expected vaporization. Early results on comet Kohoutek suggest that the conclusions could be slightly different for some of the new comets in Oort's sense. If the far ultraviolet observations confirm the early assessments of the production rates of C, O an...
A variety of physical and chemical processes are important in the comae of active comets near the Su...
Interpretation of the volatile abundances in Halley's comet in terms of models for chemical and phys...
Comets are one of our most direct links to the conditions present in the early Solar System. They h...
International audienceComets are expected to be the most primitive objects in the Solar System. The ...
International audienceComets are expected to be the most primitive objects in the Solar System. The ...
International audienceComets are expected to be the most primitive objects in the Solar System. The ...
A computer model of comet comae is described; results from assumed composition of frozen gases are s...
peer reviewedThe recent observations show that comet C/2016 R2 (Pan-Starrs) has a unique and peculia...
peer reviewedThe recent observations show that comet C/2016 R2 (Pan-Starrs) has a unique and peculia...
Context. The Rosetta encounter with comet 67P/Churyumov-Gerasimenko provides a unique opportunity fo...
Context. The Rosetta encounter with comet 67P/Churyumov-Gerasimenko provides a unique opportunity fo...
International audienceComets are low-density, kilometer-sized bodies of ices (mostly H2O, CO2, and C...
International audienceComets are low-density, kilometer-sized bodies of ices (mostly H2O, CO2, and C...
International audienceComets are low-density, kilometer-sized bodies of ices (mostly H2O, CO2, and C...
A highly abridged review of new relevant results from the observations of Comet Kohoutek is followed...
A variety of physical and chemical processes are important in the comae of active comets near the Su...
Interpretation of the volatile abundances in Halley's comet in terms of models for chemical and phys...
Comets are one of our most direct links to the conditions present in the early Solar System. They h...
International audienceComets are expected to be the most primitive objects in the Solar System. The ...
International audienceComets are expected to be the most primitive objects in the Solar System. The ...
International audienceComets are expected to be the most primitive objects in the Solar System. The ...
A computer model of comet comae is described; results from assumed composition of frozen gases are s...
peer reviewedThe recent observations show that comet C/2016 R2 (Pan-Starrs) has a unique and peculia...
peer reviewedThe recent observations show that comet C/2016 R2 (Pan-Starrs) has a unique and peculia...
Context. The Rosetta encounter with comet 67P/Churyumov-Gerasimenko provides a unique opportunity fo...
Context. The Rosetta encounter with comet 67P/Churyumov-Gerasimenko provides a unique opportunity fo...
International audienceComets are low-density, kilometer-sized bodies of ices (mostly H2O, CO2, and C...
International audienceComets are low-density, kilometer-sized bodies of ices (mostly H2O, CO2, and C...
International audienceComets are low-density, kilometer-sized bodies of ices (mostly H2O, CO2, and C...
A highly abridged review of new relevant results from the observations of Comet Kohoutek is followed...
A variety of physical and chemical processes are important in the comae of active comets near the Su...
Interpretation of the volatile abundances in Halley's comet in terms of models for chemical and phys...
Comets are one of our most direct links to the conditions present in the early Solar System. They h...