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The Effect of Weak Cosmic-ray Heating Events on the Desorption of H2

The typical amount of molecular hydrogen (H _2 ) in interstellar ices is not known, but significant freeze-out of H _2 on dust grains is not expected. However, chemical models ubiquitously predict large amounts of H _2 freeze-out in dense cloud conditions, and specialized treatments are needed to co...

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Bibliografiska uppgifter
Huvudupphov: Olli Sipilä, Kedron Silsbee, Naomi Carbajal, Paola Caselli, Marco Padovani
Materialtyp: Artigo
Språk:Inglês
Utgiven: IOP Publishing 2025-01-01
Serie:The Astrophysical Journal
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Länkar:https://doi.org/10.3847/1538-4357/adec8f
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