Details

Autor(en) / Beteiligte

• Acharyya, K.
• Fuchs, G. W.
• Fraser, H. J.
• van Dishoeck, E. F.
• Linnartz, H.

Titel

Desorption of CO and O2 interstellar ice analogs

Ist Teil von

• Astronomy and astrophysics (Berlin), 2007-05, Vol.466 (3), p.1005-1012

Ort / Verlag

Les Ulis: EDP Sciences

Erscheinungsjahr

2007

Link zum Volltext

Quelle

EZB Electronic Journals Library

Beschreibungen/Notizen

• Aims.Solid O2 has been proposed as a possible reservoir for molecular oxygen in dense clouds through freeze-out processes. The aim of this work is to characterize quantitatively the physical processes that are involved in the desorption kinetics of CO–O2 ices by interpreting laboratory temperature programmed desorption (TPD) data. This information is used to simulate the behavior of CO–O2 ices under astrophysical conditions. Methods.The TPD spectra have been recorded under ultra high vacuum conditions for pure, layered and mixed morphologies for different thicknesses, temperatures and mixing ratios. An empirical kinetic model is used to interpret the results and to provide input parameters for astrophysical models. Results.Binding energies are determined for different ice morphologies. Independent of the ice morphology, the desorption of O2 is found to follow 0th-order kinetics. Binding energies and temperature-dependent sticking probabilities for CO–CO, O2–O2 and CO–O2 are determined. O2 is slightly less volatile than CO, with a binding energy of $912\pm15$ versus $858\pm15$ K for pure ices. In mixed and layered ices, CO does not co-desorb with O2 but its binding energy is slightly increased compared to pure ice whereas that of O2 is slightly decreased. Lower limits to the sticking probabilities of CO and O2 are 0.9 and 0.85, respectively, at temperatures below 20 K. The balance between accretion and desorption is studied for O2 and CO in astrophysically relevant scenarios. Only minor differences are found between the two species, i.e., both desorb between 16 and 18 K in typical environments around young stars. Thus, clouds with significant abundances of gaseous CO are unlikely to have large amounts of solid O2.