Chemistry in disks - IV. Benchmarking gas-grain chemical models with surface reactions
A&A, 522 (2010) A42
Published online: 2010-10-29
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The efficiency of photodissociation for molecules in interstellar ices
J KalvānsMonthly Notices of the Royal Astronomical Society 478 (2) 2753 (2018)
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Physical properties and chemical composition of the cores in the California molecular cloud
Guo-Yin Zhang, Jin-Long Xu, A. I. Vasyunin, et al.Astronomy & Astrophysics 620 A163 (2018)
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Predicting HCN, HCO+, multi-transition CO, and dust emission of star-forming galaxies
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A detailed framework to incorporate dust in hydrodynamical simulations
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Large-scale Spectroscopic Mapping of the ρ Ophiuchi Molecular Cloud Complex. I. The C2H-to-N2H+ Ratio as a Signpost of Cloud Characteristics
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On the methanol emission detection in the TW Hya disc: the role of grain surface chemistry and non-LTE excitation
S. Yu. Parfenov, D. A. Semenov, Th. Henning, et al.Monthly Notices of the Royal Astronomical Society 468 (2) 2024 (2017)
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Grain Surface Models and Data for Astrochemistry
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A Surface Density Perturbation in the TW Hydrae Disk at 95 au Traced by Molecular Emission
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