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Titlebook: Experiments on Cosmic Dust Analogues; Proceedings of the S Ezio Bussoletti,Carlo Fusco,Giuseppe Longo Conference proceedings 1988 Kluwer Ac

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樓主: Buren
11#
發(fā)表于 2025-3-23 12:28:17 | 只看該作者
12#
發(fā)表于 2025-3-23 14:27:15 | 只看該作者
Nanoparticles in Biomedical Applications,essential for the optical properties of the medium because they can condense and make solids or large molecules which have optical wide bands whereas atom ions or small molecules (H, H., He, H....) only have narrow lines and cannot give a continuous absorption in a large range of wavelengths.
13#
發(fā)表于 2025-3-23 21:22:54 | 只看該作者
Shilpi Srivastava,Atul Bhargavaorphous material, takes place by itself due to the combined action of temperature and time and thus does not present experimental problems. Because of its spontaneous decay, the amorphous state is metastable and the conversion to the crystalline phase at a given temperature may take seconds or billi
14#
發(fā)表于 2025-3-24 00:22:36 | 只看該作者
15#
發(fā)表于 2025-3-24 06:25:43 | 只看該作者
16#
發(fā)表于 2025-3-24 09:09:46 | 只看該作者
Conference proceedings 1988ons are mostly lacking. It appeared then very tempting to gather together experimentalists, ob- servers and theoreticians working in the field of cosmic dust and in related areas. The Workshop held in Capri (Italy) from September 8th till 12th 1987 gave the participants a unique opportunity for exch
17#
發(fā)表于 2025-3-24 14:43:56 | 只看該作者
Semra Unal,Oguzhan Gunduz,Muhammet Uzun a limited facet of experiments on grain analogs and does not generally treat the different technique in great depth. The references take care of this deficiency. In the silicate working group, particular aspects could be considered more critically and in greater detail.
18#
發(fā)表于 2025-3-24 18:33:01 | 只看該作者
19#
發(fā)表于 2025-3-24 21:52:03 | 只看該作者
Ali Haider,Muhammad Ikram,Asma Rafiqsome major questions remain still controversial. According Mathis (1986a) it is crucial to note that the words “interstellar dust” refer to different materials as soon as we consider different space regions as the diffuse ISM, the outer edges of dense clouds, the dark central regions of these clouds.
20#
發(fā)表于 2025-3-25 00:28:18 | 只看該作者
Shilpi Srivastava,Atul Bhargavaons of years depending on the activation energy involved. For the silicates which are of interest here, the transition takes place within a reasonable amount of time at temperature in the order of 500 to 1000°C.
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