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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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发表于 2025-3-21 19:38:54 | 显示全部楼层 |阅读模式
书目名称Comets to Cosmology
副标题Proceedings of the T
编辑Andrew Lawrence
视频videohttp://file.papertrans.cn/231/230146/230146.mp4
丛书名称Lecture Notes in Physics
图书封面Titlebook: Comets to Cosmology; Proceedings of the T Andrew Lawrence Conference proceedings 1988 Springer-Verlag Berlin Heidelberg 1988 Redshift.aster
描述These proceedings are concerned with discoveries from the Infra-Red Astronomical Satellite IRAS including follow-up projects in theoretical and observational astronomy. In particular, they stress the solar system results from IRAS. A huge range of astronomical topics is addressed including asteroids, comets, dust in the solar neighbourhood, young stars, old stars, the interstellar medium, and the Galactic cosmic background at various wavelengths.
出版日期Conference proceedings 1988
关键词Redshift; asteroid; astronomy; cosmic microwave background; cosmology; solar system; star; star formation
版次1
doihttps://doi.org/10.1007/BFb0118781
isbn_ebook978-3-540-39067-1Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 1988
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发表于 2025-3-21 22:39:49 | 显示全部楼层
The infrared spectrum of Comet P/Halley,ed and the unsaturated form, with a total number of carbon atoms equal to about 30 % of H.O. With this result it is possble to define a cometary composition which is in global agreement with the composition found for interstellar dust.
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Infrared cirrus,es such as polycyclic aromatic molecules which are heated for short periods by single photons..The structure and brightness of these cirrus clouds are such that they will be a limitation to the sensitivity of future space observatories in the far infrared.
发表于 2025-3-22 06:45:27 | 显示全部楼层
0075-8450 asteroids, comets, dust in the solar neighbourhood, young stars, old stars, the interstellar medium, and the Galactic cosmic background at various wavelengths.978-3-540-39067-1Series ISSN 0075-8450 Series E-ISSN 1616-6361
发表于 2025-3-22 10:37:00 | 显示全部楼层
https://doi.org/10.1007/978-3-531-92819-7tion and modeling of the zodiacal emission. Current models provide a reasonable basis for study of the interplanetary dust, but are severely stressed when one wishes to know the ‘residual’ sky brightness. The nature, status, and implications of various models are reviewed.
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https://doi.org/10.1007/978-3-531-92819-7suggest that the outer edge is located near the edge of the asteroid belt, that the grains absorb and radiate like blackbodies, and that the density is consistent with Poynting-Robertson drag on grains originating in the asteroid belt.
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