標題: Titlebook: Cosmic Chemistry; Gerhard Klare Conference proceedings 1988 Springer-Verlag Berlin Heidelberg 1988 astrophysics.galaxies.interstellar matt [打印本頁] 作者: EFFCT 時間: 2025-3-21 17:42
書目名稱Cosmic Chemistry影響因子(影響力)
書目名稱Cosmic Chemistry影響因子(影響力)學(xué)科排名
書目名稱Cosmic Chemistry網(wǎng)絡(luò)公開度
書目名稱Cosmic Chemistry網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Cosmic Chemistry被引頻次
書目名稱Cosmic Chemistry被引頻次學(xué)科排名
書目名稱Cosmic Chemistry年度引用
書目名稱Cosmic Chemistry年度引用學(xué)科排名
書目名稱Cosmic Chemistry讀者反饋
書目名稱Cosmic Chemistry讀者反饋學(xué)科排名
作者: Fulminate 時間: 2025-3-21 21:25 作者: 排出 時間: 2025-3-22 03:12
Vertical Profiles Over Flat Terrain, of genuine solar material important clues about our heliosphere and its history as well as about “our” star in relation with other stars may be found. However, there is still an embarrassing scarcity of conclusive data, because of problems not only with instrumentation but also with data interpretation.作者: Chronic 時間: 2025-3-22 05:05 作者: champaign 時間: 2025-3-22 11:05
Chemical Composition and Ionisation States of the Solar Wind Plasma as Characteristics of Solar Phe of genuine solar material important clues about our heliosphere and its history as well as about “our” star in relation with other stars may be found. However, there is still an embarrassing scarcity of conclusive data, because of problems not only with instrumentation but also with data interpretation.作者: 易怒 時間: 2025-3-22 16:49
https://doi.org/10.1007/978-3-642-74188-3astrophysics; galaxies; interstellar matter; milky way; solar wind; telescope作者: 易怒 時間: 2025-3-22 17:40
978-3-642-74190-6Springer-Verlag Berlin Heidelberg 1988作者: ciliary-body 時間: 2025-3-23 00:18 作者: 清晰 時間: 2025-3-23 02:34 作者: BOGUS 時間: 2025-3-23 07:23
Turn Ah-Ha Moments into Pivotal Learning,lution and nucleosynthesis as well as the chemical and dynamical evolution of the Galaxy. The basic transport mechanisms in stellar atmospheres rule the . aspects of stellar surfaces which are manifest in stellar spectra. They involve radiation hydrodynamics, convection, and diffusion, and they must作者: 細菌等 時間: 2025-3-23 10:32 作者: 一美元 時間: 2025-3-23 16:03
Turn Ah-Ha Moments into Pivotal Learning,bsorption and scattering of visible radiation as well as from emission at longer wavelengths. In particular, radioastronomical and, to a lesser extent, infrared observations have helped to uncover the existence of vast interstellar clouds of gaseous and particulate matter, with most of the matter (≈作者: barium-study 時間: 2025-3-23 19:19 作者: 頭盔 時間: 2025-3-24 00:12 作者: HUMP 時間: 2025-3-24 02:42 作者: 財主 時間: 2025-3-24 10:05
Vertical Profiles Over Flat Terrain,nd square degrees was completed less than one year ago by DAME et al. [1]. Two 1.2m radio telescopes, one located in New York City, the other in Chile, were used to sample about 7700 deg. with the angular resolution degraded to 0.5° in order to cover large areas quickly. Other surveys used significa作者: 殘廢的火焰 時間: 2025-3-24 11:19 作者: oxidize 時間: 2025-3-24 18:10
Qinghe Dong,Qian He,Mengfei Cai,Peng Liurelevant time scales shows that nonequilibrium effects have to be taken into account. In order to demonstrate these non-equilibrium effects, the detailed chemical structure of the shell of α-Ori has been calculated with the physical and chemical parameters taken from CLEGG et al.[1]. The correspondi作者: Odyssey 時間: 2025-3-24 19:27
Zhou Chen,Qi Qi,Changjun Wang,Wenwei WangSome 4.6 billion years ago contraction and subsequent collapse of an interstellar cloud led to the formation of the solar system. The ratio of heavy elements to hydrogen, increasing continuously in interstellar material, due to the addition of freshly synthesized material from stars, was frozen in for the solar system at this point of time.作者: Orthodontics 時間: 2025-3-25 00:46 作者: Interim 時間: 2025-3-25 04:09 作者: florid 時間: 2025-3-25 11:21 作者: diathermy 時間: 2025-3-25 12:14
Interstellar Molecular Formation Processes,a, the gaseous molecules are exceedingly well characterized and their observation leads to a detailed knowledge of the chemical and physical state of the gas in dense interstellar clouds [2, 3]. For example, gas temperatures are in the range 10 – 70 K and total gas densities are on the order of 10. 作者: 膽小鬼 時間: 2025-3-25 18:01
Nonequilibrium Chemistry in Circumstellar Shells,nstant outflow velocity of 10 km/s, the H. concentration shows the most pronounced departure from kinetic equilibrium caused by the specific temperature-dependence of the main H.-forming reactions and by wind effects. Periodic oscillations of UV radiation and temperature cause a significant departur作者: Osteons 時間: 2025-3-25 21:38
Turn Ah-Ha Moments into Pivotal Learning,a, the gaseous molecules are exceedingly well characterized and their observation leads to a detailed knowledge of the chemical and physical state of the gas in dense interstellar clouds [2, 3]. For example, gas temperatures are in the range 10 – 70 K and total gas densities are on the order of 10. 作者: 除草劑 時間: 2025-3-26 04:06 作者: 神圣在玷污 時間: 2025-3-26 06:56 作者: 鞏固 時間: 2025-3-26 09:20 作者: 轉(zhuǎn)換 時間: 2025-3-26 16:01 作者: 串通 時間: 2025-3-26 18:37 作者: 有毛就脫毛 時間: 2025-3-26 22:26 作者: 外形 時間: 2025-3-27 05:09 作者: 問到了燒瓶 時間: 2025-3-27 08:49 作者: 強行引入 時間: 2025-3-27 09:43
0941-1445 astrophysics. The twelve contributions to this book, written by experts from the US, UK, France, Belgium, Switzerland and Germany, deal in depth with the chemistry of comets and meteorites, of stars and their shells, of the interstellar medium and galaxies. A comprehensive review of nucleosynthesis作者: Curmudgeon 時間: 2025-3-27 16:02
Vertical Profiles Over Flat Terrain,, were used to sample about 7700 deg. with the angular resolution degraded to 0.5° in order to cover large areas quickly. Other surveys used significantly higher angular resolution but have been limited to selected nearby molecular clouds and a thin strip covering the inner galactic plane. The most extensive of these surveys are:作者: 笨拙處理 時間: 2025-3-27 18:52 作者: 厚顏無恥 時間: 2025-3-28 01:29 作者: Rotator-Cuff 時間: 2025-3-28 02:07
Vertical Profiles Over Flat Terrain, ≈ 82 and 50 neighbours, may be sufficient to explain the observed r-abundances in the A ≈ 130 and 80 abundance peaks. Based on this result, new constraints are given on the stellar conditions under which a steady-flow r-process has operated.作者: 鞭子 時間: 2025-3-28 08:47 作者: 灌輸 時間: 2025-3-28 13:34
,Nuclear Physics Constraints to Bring the Astrophysical R-Process to the “Waiting Point”, ≈ 82 and 50 neighbours, may be sufficient to explain the observed r-abundances in the A ≈ 130 and 80 abundance peaks. Based on this result, new constraints are given on the stellar conditions under which a steady-flow r-process has operated.作者: Outwit 時間: 2025-3-28 15:35 作者: Bronchial-Tubes 時間: 2025-3-28 20:24 作者: 北京人起源 時間: 2025-3-29 00:54
,Composition in Halley’s Comet: Clues to Origin and History of Cometary Matter, found in the smaller objects of the solar system. We present estimates for molecular and elemental abundances in the material released by Halley’s comet. They are based on data of the gas and dust composition in the coma. Highly volatile material is very abundant, consistent with condensation and a作者: 輕快走過 時間: 2025-3-29 05:08 作者: Engaged 時間: 2025-3-29 10:14
Chemistry of Circumstellar Shells, for their chemistry, and the observed molecular abundances. The discussion of the chemistry of layers just above the photosphere is very difficult because of their complexity. Modeling of radical and ion photochemistry is now successful in accounting for the observed species, often complex, observe作者: CRUE 時間: 2025-3-29 13:33
Interstellar Molecular Formation Processes,bsorption and scattering of visible radiation as well as from emission at longer wavelengths. In particular, radioastronomical and, to a lesser extent, infrared observations have helped to uncover the existence of vast interstellar clouds of gaseous and particulate matter, with most of the matter (≈作者: 激怒 時間: 2025-3-29 16:08 作者: 刺激 時間: 2025-3-29 20:17
Chemical Composition and Ionisation States of the Solar Wind Plasma as Characteristics of Solar Phe of genuine solar material important clues about our heliosphere and its history as well as about “our” star in relation with other stars may be found. However, there is still an embarrassing scarcity of conclusive data, because of problems not only with instrumentation but also with data interpreta作者: cluster 時間: 2025-3-30 03:14 作者: Munificent 時間: 2025-3-30 07:52
Molecular Clouds in the Milky Way: the Columbia-Chile CO Survey and Detailed Studies with the KOSMAnd square degrees was completed less than one year ago by DAME et al. [1]. Two 1.2m radio telescopes, one located in New York City, the other in Chile, were used to sample about 7700 deg. with the angular resolution degraded to 0.5° in order to cover large areas quickly. Other surveys used significa
