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Titlebook: European Conference on Laboratory Astrophysics ECLA2020; The Interplay of Dus Vito Mennella,Christine Joblin Conference proceedings 2023 Th

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31#
發(fā)表于 2025-3-27 00:29:17 | 只看該作者
The Nanocosmos Receivers for?Laboratory Astrophysics and?Radioastronomical Observations: GACELA and xtremely sensitive receivers, allowing the discovery of more than 30 new molecular species, including eight cations, one anion, seven neutral S-bearing species, radicals, and a large number of hydrocarbons including the first identification of a non functionalized polycyclic aromatic hydrocarbon in space, indene (C.H.).
32#
發(fā)表于 2025-3-27 03:36:35 | 只看該作者
33#
發(fā)表于 2025-3-27 08:33:09 | 只看該作者
Late-Type Stars Seen at?High Spectral Resolution at?Mid-Infrared Wavelengthsther progress. Our laboratory mid-IR high-resolution experimental setup is presented and examples of investigated molecules, like TiO and Al.O are given. We also describe observations of late-type stars using the TEXES spectrograph on the NASA Infrared Telescope Facility (IRTF).
34#
發(fā)表于 2025-3-27 11:00:33 | 只看該作者
Physics and?Chemistry of?PhotoDissociation Regionstion of H. as well as the role of large molecules in the photo-electric heating and chemical composition of the gas. I will also review the chemical evolution of Polycyclic Aromatic Hydrocarbon molecules driven by photo-dissociation and isomerization processes. Relevant laboratory studies and quantum chemical calculations will be pointed out.
35#
發(fā)表于 2025-3-27 15:32:29 | 只看該作者
36#
發(fā)表于 2025-3-27 17:51:39 | 只看該作者
37#
發(fā)表于 2025-3-27 23:04:44 | 只看該作者
38#
發(fā)表于 2025-3-28 02:45:01 | 只看該作者
Conference proceedings 2023, physicists, chemists, and geophysicists. It provides an update on outstanding results in this research field, the presentation of new laboratory developments, and the recent and expected to come space missions and other astronomical observatories with their specific needs for laboratory and theore
39#
發(fā)表于 2025-3-28 08:31:46 | 只看該作者
Psychotherapie und Geschlechtszugeh?rigkeitthe radicals upon encounter, namely on the water ice structure and interaction of the two radicals. These results indicate that the fraction of iCOMs generated in the current astrochemical models is certainly overestimated since (i) it is assumed that iCOM forming reactions always occur and (ii) the competitive reactions are often not included.
40#
發(fā)表于 2025-3-28 12:16:04 | 只看該作者
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