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

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書(shū)目名稱Comets to Cosmology影響因子(影響力)




書(shū)目名稱Comets to Cosmology影響因子(影響力)學(xué)科排名




書(shū)目名稱Comets to Cosmology網(wǎng)絡(luò)公開(kāi)度




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書(shū)目名稱Comets to Cosmology被引頻次學(xué)科排名




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書(shū)目名稱Comets to Cosmology年度引用學(xué)科排名




書(shū)目名稱Comets to Cosmology讀者反饋




書(shū)目名稱Comets to Cosmology讀者反饋學(xué)科排名

Mortal

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

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.

充滿人

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

vibrant

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

guzzle

Chameleon

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使出神

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.