corrode
发表于 2025-3-21 19:38:54
书目名称Comets to Cosmology影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0230146<br><br> <br><br>书目名称Comets to Cosmology影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0230146<br><br> <br><br>书目名称Comets to Cosmology网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0230146<br><br> <br><br>书目名称Comets to Cosmology网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0230146<br><br> <br><br>书目名称Comets to Cosmology被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0230146<br><br> <br><br>书目名称Comets to Cosmology被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0230146<br><br> <br><br>书目名称Comets to Cosmology年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0230146<br><br> <br><br>书目名称Comets to Cosmology年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0230146<br><br> <br><br>书目名称Comets to Cosmology读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0230146<br><br> <br><br>书目名称Comets to Cosmology读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0230146<br><br> <br><br>
Mortal
发表于 2025-3-21 22:39:49
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.
intolerance
发表于 2025-3-22 00:25:19
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.
充满人
发表于 2025-3-22 06:45:27
0075-8450asteroids, 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
vibrant
发表于 2025-3-22 10:37:00
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.
guzzle
发表于 2025-3-22 15:24:42
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guzzle
发表于 2025-3-22 20:31:00
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Chameleon
发表于 2025-3-23 00:41:33
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开始没有
发表于 2025-3-23 03:30:49
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使出神
发表于 2025-3-23 09:26:25
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.