Symposium - International Astronomical Union, Molecules in Astrophysics: Probes and Processes
- This volume was published under a former title. See this journal's title history.
Basic Molecular Processes
In Memoriam: Sheldon Green
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- 25 May 2016, pp. 239-240
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Inelastic collisions of interstellar molecules: Experiment Versus Theory
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- 25 May 2016, pp. 241-252
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Reactions between neutral species at low temperatures: Laboratory results and astrophysical modelling
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- 25 May 2016, pp. 253-270
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Dynamics of chemical reactions of astrophysical interest
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- 25 May 2016, pp. 271-280
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Infrared and optical spectroscopy of astrophysical molecules
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- 25 May 2016, pp. 281-286
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Electronic spectra of carbon chains of relevance to astrophysics
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- 25 May 2016, pp. 287-294
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Determination of opacity data bases for TiO and H2O
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- 25 May 2016, pp. 295-303
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Microprobe two-step laser mass spectrometry as an analytical tool for meteoritic samples
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- 25 May 2016, pp. 305-320
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Modeling of interstellar surface processes: What does the surface of grains look like?
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- 25 May 2016, pp. 321-330
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Laboratory simulation of physical and chemical processes in interstellar ices
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- 25 May 2016, pp. 331-340
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Grains and Pahs
Interstellar dust grains - an overview
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- 25 May 2016, pp. 343-356
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The PAH Hypothesis: Spectroscopic properties of large aromatic molecules in the infrared
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- 25 May 2016, pp. 357-366
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New dust features in oxygen-rich envelopes
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- 25 May 2016, pp. 367-370
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ISO First Results
Infrared spectroscopy with the Infrared Space Observatory
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- 25 May 2016, pp. 373-384
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Detection of thermal water vapor emission from W Hydrae
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- 25 May 2016, pp. 385-388
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ISO LWS spectra of AGB and post-AGB objects
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- 25 May 2016, pp. 389-392
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First detection of thermal H2O Emission from a Herbig-Haro Object
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- 25 May 2016, pp. 393-396
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Abundant, hot water toward young stellar objects
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- 25 May 2016, pp. 397-400
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A search for interstellar gas-phase CO2
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- 25 May 2016, pp. 401-404
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Diffuse and Translucent Clouds
Optical and ultraviolet observations of diffuse interstellar clouds
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- 25 May 2016, pp. 407-420
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