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Titlebook: Chemistry in Space; J. M. Greenberg,V. Pirronello Book 1991 Kluwer Academic Publishers 1991 LOPES.Supernova.collision.cosmic ray.interstel

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51#
發(fā)表于 2025-3-30 08:50:52 | 只看該作者
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發(fā)表于 2025-3-30 14:25:33 | 只看該作者
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發(fā)表于 2025-3-30 18:13:43 | 只看該作者
Book 1991pace was indeed a surprise considering that only a short time ear- lier there were still arguments about the existence of the simplest of all molecules - the hydrogen molecule. The application of ion-molecule reactions to interstellar cloud chemistry provided a rich variety of new possibilities whic
54#
發(fā)表于 2025-3-30 21:50:51 | 只看該作者
Paul Michael Brannagan,Danyel Reicheceptionally close to the Sun); CSEs are the most obvious location of formation of cosmic dust grains, with fascinating, albeit complex, processes of dust formation and interaction with the gas, and also the possibility that interstellar and solar system solid particles keep a memory of the circumste
55#
發(fā)表于 2025-3-31 04:25:13 | 只看該作者
Tzvetan S. Metodi,Frederic T. Chongresence of organic compounds similar to observed in carbonaceous chondrites. The results of cometary dust composition measurements shows to a possible similarity of interstellar and cometary dust and can be explained by a model of cometary nuclei as aggregates of interstellar dust particles with no
56#
發(fā)表于 2025-3-31 07:03:58 | 只看該作者
57#
發(fā)表于 2025-3-31 10:06:46 | 只看該作者
Features of Experimental Studying of Comet Halley Dust Particles Elemental Compositionresence of organic compounds similar to observed in carbonaceous chondrites. The results of cometary dust composition measurements shows to a possible similarity of interstellar and cometary dust and can be explained by a model of cometary nuclei as aggregates of interstellar dust particles with no
58#
發(fā)表于 2025-3-31 15:29:16 | 只看該作者
1389-2185 l molecules - the hydrogen molecule. The application of ion-molecule reactions to interstellar cloud chemistry provided a rich variety of new possibilities whic978-94-010-6798-0978-94-009-0695-2Series ISSN 1389-2185
59#
發(fā)表于 2025-3-31 18:19:43 | 只看該作者
60#
發(fā)表于 2025-4-1 01:09:56 | 只看該作者
The Molecular Composition of Dense Interstellar Cloudson and chemical evolution are, in consequence, fundamental aspects of nature whose investigation is basic to space chemistry. Because the physical conditions in these clouds are quite extreme by the standards of the terrestrial laboratory, they provide a chemical environment which is quite different
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