Reference : Hydrates de gaz dans les noyaux cométaires et les grains interstellaires
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/71711
Hydrates de gaz dans les noyaux cométaires et les grains interstellaires
French
Delsemme, A.-H. [Université de Liège - ULg > Institut d'Astrophysique de Liège > > > >]
Swings, Polydore [Université de Liège - ULg > Institut d'Astrophysique de Liège > > > >]
1952
Annales d'astrophysique
Caisse nationale de la recherche scientifique
15
1
1-6
No
International
0365-0499
Paris
France
[en] Solid hydrates of CH4, CO2, ... may be present in cometary nuclei and interstellar grains. The vapor pressures — hence the rates of sublimation — of the various hydrates are of the same order of magnitude while the vapor pressures of solid CH4, H2O, ... differ by very large factors. The relative abundances of the radicals which are observed in comets would be explained more satisfactorily by assuming the presence of solid hydrates.
Researchers ; Professionals
http://hdl.handle.net/2268/71711
http://adsabs.harvard.edu/abs/1952AnAp...15....1D

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