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Titlebook: Comets to Cosmology; Proceedings of the T Andrew Lawrence Conference proceedings 1988 Springer-Verlag Berlin Heidelberg 1988 Redshift.aster

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樓主: corrode
51#
發(fā)表于 2025-3-30 11:35:25 | 只看該作者
Christian Seelos,Kate Ganly,Johanna Mairnd albedo of ~0.05. It is inferred that the nucleus itself is dark. Upper limits on the number density of trail particles are calulated. The mean free path between trail particles suggests that the Comet Rendevous/Asteroid Flyby mission is unlikely to be affected if it flies within the trail ahead o
52#
發(fā)表于 2025-3-30 16:00:24 | 只看該作者
Social Enterprise Theoretical Framework,a physical model that describes at the four IRAS wavelengths the contaminating contribution of the zodiacal emission. Direct comparison between the 100 . and HI column density maps shows a good correlation at high galactic latitudes. After radial unfolding the 12, 25, 60 and 100 . radial profiles ar
53#
發(fā)表于 2025-3-30 19:06:11 | 只看該作者
https://doi.org/10.1007/978-3-319-01396-1 used as a very rigid observational constraint of the model. It is found that dust associated with atomic hydrogen is the dominant contribution to the total infrared luminosity. Correlations between warm and cold dust emission. HII regions and the distribution of the atomic gas are analyzed. Dust pr
54#
發(fā)表于 2025-3-30 23:57:17 | 只看該作者
55#
發(fā)表于 2025-3-31 03:00:51 | 只看該作者
56#
發(fā)表于 2025-3-31 06:47:58 | 只看該作者
The Challenge of Public Goods Provisionhe origin of the infrared emission from the solar neigbourhood. We show that altough most of the emission comes from interstellar matter not associated with current star formation, about half of the heating of grains is provided by ultraviolet photons radiated by stars younger than few 10. yrs.
57#
發(fā)表于 2025-3-31 11:30:18 | 只看該作者
58#
發(fā)表于 2025-3-31 13:55:08 | 只看該作者
59#
發(fā)表于 2025-3-31 18:51:05 | 只看該作者
60#
發(fā)表于 2025-4-1 01:34:16 | 只看該作者
https://doi.org/10.1007/BFb0118781Redshift; asteroid; astronomy; cosmic microwave background; cosmology; solar system; star; star formation
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