Cosmic Ray Compaction of Porous Interstellar Ices

We studied the compaction of microporous vapor-deposited ice films under irradiation with different ions in the 80-400 keV energy range. We found that porosity decreases exponentially with irradiation fluence, with a mean compaction area per ion that scales linearly with the stopping power of the pr...

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Veröffentlicht in:The Astrophysical journal 2008-11, Vol.687 (2), p.1070-1074
Hauptverfasser: Raut, U, Famá, M, Loeffler, M. J, Baragiola, R. A
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Sprache:eng
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Zusammenfassung:We studied the compaction of microporous vapor-deposited ice films under irradiation with different ions in the 80-400 keV energy range. We found that porosity decreases exponentially with irradiation fluence, with a mean compaction area per ion that scales linearly with the stopping power of the projectile S above a threshold [image] eV Aa super(-1). The experiments roughly follow a universal dependence of ion-induced compaction with restricted dose (eV molecule super(-1)). This behavior can be used to extrapolate our results to conditions of the interstellar medium. Relating our results to ionization rates of interstellar H sub(2), we estimate that porous ice mantles on grains in dense molecular clouds are compacted by cosmic rays in [image]10-50 million years.
ISSN:0004-637X
1538-4357
DOI:10.1086/592193