Interstellar dust
Interstellar dust
Interstellar dust
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Results<br />
Grains 10 K favours hydrogenation<br />
Warmer grains (30 K) favours oxygenation<br />
UV photons dissociate species that recombine. “dissociationformation-dissociation”<br />
boost gas phase.<br />
P free<br />
Etc.<br />
Species released in gas photo-dissociated.<br />
Boost VS photo-dissociation?