標(biāo)題: Titlebook: ISO Science Legacy; A Compact Review of Catherine Cesarsky,Alberto Salama Book 2005 Springer Science+Business Media B.V. 2005 Galaxy.Quasa [打印本頁] 作者: informed 時(shí)間: 2025-3-21 16:11
書目名稱ISO Science Legacy影響因子(影響力)
書目名稱ISO Science Legacy影響因子(影響力)學(xué)科排名
書目名稱ISO Science Legacy網(wǎng)絡(luò)公開度
書目名稱ISO Science Legacy網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱ISO Science Legacy被引頻次
書目名稱ISO Science Legacy被引頻次學(xué)科排名
書目名稱ISO Science Legacy年度引用
書目名稱ISO Science Legacy年度引用學(xué)科排名
書目名稱ISO Science Legacy讀者反饋
書目名稱ISO Science Legacy讀者反饋學(xué)科排名
作者: 低能兒 時(shí)間: 2025-3-21 22:45 作者: STYX 時(shí)間: 2025-3-22 01:23 作者: Culpable 時(shí)間: 2025-3-22 07:47 作者: multiply 時(shí)間: 2025-3-22 11:15 作者: Indent 時(shí)間: 2025-3-22 13:34
978-90-481-6979-5Springer Science+Business Media B.V. 2005作者: dainty 時(shí)間: 2025-3-22 17:05
be, and has been kept in most subtribes except for Ditomina. In this subtribe high numbers around 2n = 57 (2n = 45?69) are found. The origin of these high numbers is discussed and it is concluded that karyotypic, geographical, and behavioural peculiarities justify the ranking of Ditomina as an indep作者: HOWL 時(shí)間: 2025-3-23 01:10 作者: 緯線 時(shí)間: 2025-3-23 02:12 作者: cunning 時(shí)間: 2025-3-23 09:29
Thomas G. Müller,Péter ábrahám,Jacques Crovisiern materials processing since they do not involve the tedious steps and large, environmentally burdensome, liquid volumes of wet chemical processes. In addition, the time scales of aerosol processes are much shorter than those involving solid-solid reactions. Furthermore, these processes can produce 作者: 天氣 時(shí)間: 2025-3-23 13:18
n materials processing since they do not involve the tedious steps and large, environmentally burdensome, liquid volumes of wet chemical processes. In addition, the time scales of aerosol processes are much shorter than those involving solid-solid reactions. Furthermore, these processes can produce 作者: 索賠 時(shí)間: 2025-3-23 17:19
Brunella Nisini,Anlaug Amanda Kaas,Ewine F. van Dishoeck,Derek Ward-Thompsonn materials processing since they do not involve the tedious steps and large, environmentally burdensome, liquid volumes of wet chemical processes. In addition, the time scales of aerosol processes are much shorter than those involving solid-solid reactions. Furthermore, these processes can produce 作者: Decibel 時(shí)間: 2025-3-23 20:40 作者: 神化怪物 時(shí)間: 2025-3-24 00:05
Marie Jourdain de Muizonn materials processing since they do not involve the tedious steps and large, environmentally burdensome, liquid volumes of wet chemical processes. In addition, the time scales of aerosol processes are much shorter than those involving solid-solid reactions. Furthermore, these processes can produce 作者: 火花 時(shí)間: 2025-3-24 03:38 作者: 無所不知 時(shí)間: 2025-3-24 07:54
Els Peeters,Nieves Leticia Martín-Hernández,Memesio J. Rodríguez-Fernández,Xander Tielenserage 1 in 20–25 α-(1,4)-bond glucose units is branched by an α-(1,6)-.-glucosidic bond. Amylose (mol wt 10.–10.) consists of much longer linear chains of which on average one in several hundred α-(1,4)-bond glucose units is branched by an α-(1,6)-.-glucosidic bond (.). The hydrolysis of starch to l作者: ANTI 時(shí)間: 2025-3-24 13:22 作者: HEDGE 時(shí)間: 2025-3-24 16:02
Conformational analysis of oligosaccharides makes the three dimensional structure available. The analysis of the conformation of oligosaccharides is usually determined by a combination of computational methods and experimental techniques. NMR spectroscopy is the most important experimental tool. The作者: Cervical-Spine 時(shí)間: 2025-3-24 21:39 作者: 一小塊 時(shí)間: 2025-3-25 01:22
Water in Space: The Water World of ISOmolecular clouds, evolved stars, galaxies, and in the bodies of our Solar System. We also discuss the modeling of H.O and the difficulties found in the interpretation of the data, the need of collisional rates and the perspectives that future high angular and high spectral resolution observations of作者: dialect 時(shí)間: 2025-3-25 03:40 作者: FECK 時(shí)間: 2025-3-25 11:24 作者: 笨重 時(shí)間: 2025-3-25 14:28 作者: panorama 時(shí)間: 2025-3-25 18:14 作者: Pageant 時(shí)間: 2025-3-25 22:11
ISO Observations of Pre-Stellar Cores and Young Stellar Objectsples of sources in different evolutionary stages are reviewed, addressing in particular how the physical and chemical properties of the proto-stellar environments change from the pre-stellar cores to the protostars at the end of their accretion phase. In addition, the mid-IR surveys in nearby star-f作者: perjury 時(shí)間: 2025-3-26 03:16
Pre-Main Sequence Stars Seen by ISObservatory (ISO) are reviewed. All the observations have been mainly carried out by using the two spectrographs SWS and LWS, adopting their low resolution modes and such data have been used both for lines detection and to reconstruct the spectral energy distributions. Line emission and photometric b作者: OGLE 時(shí)間: 2025-3-26 06:42 作者: Cholagogue 時(shí)間: 2025-3-26 08:46
Late Stages of Stellar Evolutiontalline silicates and the rotational lines of water vapour, were detected for the first time in the spectra of (post-)Asymptotic Giant Branch (AGB) stars. Their analysis has greatly improved our knowledge of stellar atmospheres and circumstellar environments. A surprising number of objects, particul作者: 偏狂癥 時(shí)間: 2025-3-26 16:22
The Cool Interstellar Mediumrstanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also the coupling between the gas and the grains. We review here the ISO results on the cool and low-excitation regions of the interstellar medium, where . .? 500 K, .H ～ 100–10. cm. and the electron d作者: 浮雕寶石 時(shí)間: 2025-3-26 19:34 作者: 熱心助人 時(shí)間: 2025-3-26 20:58
Normal Nearby Galaxies the underlying physical processes. Highlights include the discovery of an extended cold dust emission component, present in all types of gas-rich galaxies and carrying the bulk of the dust luminosity; the definitive characterisation of the spectral energy distribution in the IR, revealing the chann作者: 憲法沒有 時(shí)間: 2025-3-27 02:09 作者: organic-matrix 時(shí)間: 2025-3-27 05:45 作者: 使成核 時(shí)間: 2025-3-27 09:50
The Planets and Titan Observed by ISOon of some stratospheric hydrocarbons (CH., C.H., CH.C.H, C.H., C.H.); (5) the first detection of tropospheric water in Saturn; (6) the tentative detection of carbonate minerals on Mars; (7) the first thermal lightcurve of Pluto.作者: ADORN 時(shí)間: 2025-3-27 14:08 作者: BET 時(shí)間: 2025-3-27 19:19
Crystalline Silicatesstalline silicates is still not completely clarified, but the combination of theoretical modeling and observations have already shed light on their life-cycle. The absence of crystalline silicates in the diffuse ISM provides us with information about the dust amorphization rate in the ISM.作者: Corral 時(shí)間: 2025-3-27 22:20 作者: 巨碩 時(shí)間: 2025-3-28 05:16 作者: Munificent 時(shí)間: 2025-3-28 09:40
Comets, Asteroids and Zodiacal Light as Seen by Iso crystalline silicates, the work on asteroid surface mineralogy, results from thermophysical studies of asteroids, a new determination of the asteroid number density in the main-belt and last but not least, the investigations on the spatial and spectral features of the zodiacal light.作者: 引導(dǎo) 時(shí)間: 2025-3-28 13:13 作者: 逗它小傻瓜 時(shí)間: 2025-3-28 17:37 作者: 愛社交 時(shí)間: 2025-3-28 21:20
Late Stages of Stellar Evolutionarly young planetary nebulae with Wolf-Rayet (WR) central stars, were found to exhibit emission features in their ISO spectra that are characteristic of both oxygen-rich and carbon-rich dust species, while far-IR observations of the PDR around NGC 7027 led to the first detections of the rotational line spectra of CH and CH..作者: 混合,攙雜 時(shí)間: 2025-3-29 01:52 作者: AXIOM 時(shí)間: 2025-3-29 05:04
Book 2005ace missions and cooled telescopes, infrared astronomy is the last branch of this discipline to come of age. After a very successful sky survey performed in the eighties by the IRAS satellite, the Infrared Space Observatory, in the nineties, brought spectacular advances in the understanding of the p作者: harpsichord 時(shí)間: 2025-3-29 07:41 作者: 尊嚴(yán) 時(shí)間: 2025-3-29 14:26 作者: JEER 時(shí)間: 2025-3-29 19:28
rline. Here the communities show certain similarities to forest European ones..Comparisons between carabid coenoses over this area present considerable difficulties because of the uneven occurrence of a lot of species among the various massifs as a consequence of more colonization and extinction eve作者: 不安 時(shí)間: 2025-3-29 20:57 作者: 引水渠 時(shí)間: 2025-3-30 01:39 作者: Indicative 時(shí)間: 2025-3-30 04:25
oxides..Depending on the phase of the raw materials, aerosol processes can be classified into two routes. Powders are made at high temperatures either by reacting gases and vapors (gas-to-particle conversion route) or by transforming precursor particles/droplets to the desired product (particle-to-p作者: 安裝 時(shí)間: 2025-3-30 09:11
