標題: Titlebook: Diffuse Matter in Galaxies; Cargèse 1982 J. Audouze,J. Lequeux,A. Vidal-Madjar Book 1983 D. Reidel Publishing Company, Dordrecht, Holland 1 [打印本頁] 作者: 臉紅 時間: 2025-3-21 18:24
書目名稱Diffuse Matter in Galaxies影響因子(影響力)
書目名稱Diffuse Matter in Galaxies影響因子(影響力)學科排名
書目名稱Diffuse Matter in Galaxies網(wǎng)絡公開度
書目名稱Diffuse Matter in Galaxies網(wǎng)絡公開度學科排名
書目名稱Diffuse Matter in Galaxies被引頻次
書目名稱Diffuse Matter in Galaxies被引頻次學科排名
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書目名稱Diffuse Matter in Galaxies年度引用學科排名
書目名稱Diffuse Matter in Galaxies讀者反饋
書目名稱Diffuse Matter in Galaxies讀者反饋學科排名
作者: DAMN 時間: 2025-3-21 22:04 作者: gregarious 時間: 2025-3-22 02:01
Dynamics and Energetics of the Interstellar Medium,locks are then applied to model idealized versions of localized dynamical situations in the diffuse interstellar medium. Some observational constraints on global models of the interstellar medium are briefly discussed.作者: 考古學 時間: 2025-3-22 06:24
Recycling and trade of waste paper in Indiat review the basic knowledge of the stellar winds (Section II). The theory of the interaction between the wind and the ISM and the structure of a typical interstellar bubble (IB) from a single star is discussed in Section III. A typical example of an observed bubble, the Cygnus Superbubble, is discussed in Section IV.作者: miracle 時間: 2025-3-22 10:58 作者: Ige326 時間: 2025-3-22 16:24 作者: Ige326 時間: 2025-3-22 19:22
https://doi.org/10.1007/978-3-642-95768-0e briefly described in Section III. The evolution of the remnants is discussed in Section IV. In Section V I discuss the effect of supernovae when they occur in stellar clusters. In Section VI the overall effect of stellar winds and supernovae on the interstellar medium is described.作者: 戲服 時間: 2025-3-23 00:56 作者: 提煉 時間: 2025-3-23 05:24
1389-2185 ry) introduces the study of the diffuse interstellar medium which plays a major role in galactic evolution. His contribution provides some historical references978-94-009-7185-1978-94-009-7183-7Series ISSN 1389-2185 作者: 單獨 時間: 2025-3-23 05:36
Book 1983tions, determination of the physical properties and evolution) of this diffuse medium. In the first chapter, J. Lequeux (Marseille Observatory) introduces the study of the diffuse interstellar medium which plays a major role in galactic evolution. His contribution provides some historical references作者: synchronous 時間: 2025-3-23 13:17 作者: 假 時間: 2025-3-23 17:52 作者: 串通 時間: 2025-3-23 20:56
Grundlagen des Metallrecyclings, line formation, condensation and destruction of grains, thermal exchanges, hydrodynamic phenomena (including shocks), etc. The domain of interstellar studies is thus a carrefour of astrophysics and physics: this explains why it is presently one of the most active parts of astronomy.作者: CANT 時間: 2025-3-24 02:05
Joseph Seckbach,David J. Chapmanl gas on the evolution of the galactic disk, the use of planetary nebulae to try to deduce the rate of star formation for low mass stars etc… are reviewed. Finally the future of the studies concerning the nucleosynthesis and the chemical evolution galaxies is discussed.作者: innovation 時間: 2025-3-24 06:11 作者: Allure 時間: 2025-3-24 06:42 作者: allude 時間: 2025-3-24 12:54
Supernovae and Supernova Remnants, large that these explosions provide the dominant energy for the heating of the hot (T ? 10. K) IS component and for the kinetic energy of the large scale motions of the interstellar clouds. In addition, the ejected matter of supernovae is the main source of the chemical pollution of the IS medium. 作者: inflate 時間: 2025-3-24 16:57
Interstellar Helium and Deuterium,t elements in the universe. For both elements the different observational methods used in the interstellar medium are mentioned and the most precise ones described in more details. A discussion of the results in comparison with current theories shows that many more observations are needed. Typical f作者: faucet 時間: 2025-3-24 20:40
Nucleosynthesis and Chemical Evolution of Galaxies,s : the primordial nucleosynthesis occurring just after the Big Bang, responsible for the formation of D, .He,. He and at least in part .Li; the bombardment of the interstellar medium by galactic cosmic rays responsible for the formation of the bulk of the Li, Be, B elements; and the stellar nucleos作者: insidious 時間: 2025-3-25 02:52
Dynamics and Energetics of the Interstellar Medium,s given. Then, basic phenomena are presented: radiative losses, shocks, ionization fronts, and electron thermal conduction. These tools and building blocks are then applied to model idealized versions of localized dynamical situations in the diffuse interstellar medium. Some observational constraint作者: Highbrow 時間: 2025-3-25 03:59 作者: 人工制品 時間: 2025-3-25 10:28
Diffuse Matter in Galaxies978-94-009-7183-7Series ISSN 1389-2185 作者: stressors 時間: 2025-3-25 14:12
Brett A. Neilan,Shauna Murray,Min Chent elements in the universe. For both elements the different observational methods used in the interstellar medium are mentioned and the most precise ones described in more details. A discussion of the results in comparison with current theories shows that many more observations are needed. Typical future possibilities are suggested.作者: 玉米棒子 時間: 2025-3-25 18:48
William N. Valentine,Donald E. Pagliato charge transfer reactions, dielectronic recombination, and to photoionisation and radiative recombination. Collisional excitation of fine structure transitions by electrons and hydrogen atoms is also considered in relation to the cooling of the interstellar gas.作者: PRO 時間: 2025-3-25 21:32
Interstellar Helium and Deuterium,t elements in the universe. For both elements the different observational methods used in the interstellar medium are mentioned and the most precise ones described in more details. A discussion of the results in comparison with current theories shows that many more observations are needed. Typical future possibilities are suggested.作者: HALL 時間: 2025-3-26 02:30 作者: motivate 時間: 2025-3-26 07:55
https://doi.org/10.1007/978-94-009-7183-7Galaxy; interstellar matter; observatory; spectroscopy; stellar作者: 舊病復發(fā) 時間: 2025-3-26 12:27
978-94-009-7185-1D. Reidel Publishing Company, Dordrecht, Holland 1983作者: SIT 時間: 2025-3-26 15:46
Grundlagen des Metallrecyclings,s and dust. Stars are born from this interstellar medium and return continuously to it matter enriched in heavy elements by nucleosynthesis. Moreover exchanges of interstellar gas between different parts of a galaxy and exchanges between a galaxy, its neighbours during encounters and with the interg作者: Musket 時間: 2025-3-26 20:04
Recycling and trade of waste paper in Indiamentum of this stellar wind is so large that the wind blows a bubble into the interstellar medium (ISM). The amount of energy which is deposited into the ISM by the stellar wind during the lifetime of the star is comparable with the energy released in Supernova explosions. In this course I will firs作者: GEM 時間: 2025-3-27 01:02
https://doi.org/10.1007/978-3-642-95768-0 large that these explosions provide the dominant energy for the heating of the hot (T ? 10. K) IS component and for the kinetic energy of the large scale motions of the interstellar clouds. In addition, the ejected matter of supernovae is the main source of the chemical pollution of the IS medium. 作者: canvass 時間: 2025-3-27 04:32
Brett A. Neilan,Shauna Murray,Min Chent elements in the universe. For both elements the different observational methods used in the interstellar medium are mentioned and the most precise ones described in more details. A discussion of the results in comparison with current theories shows that many more observations are needed. Typical f作者: 斷斷續(xù)續(xù) 時間: 2025-3-27 07:24 作者: Headstrong 時間: 2025-3-27 10:12 作者: 憂傷 時間: 2025-3-27 14:44
William N. Valentine,Donald E. Pagliato charge transfer reactions, dielectronic recombination, and to photoionisation and radiative recombination. Collisional excitation of fine structure transitions by electrons and hydrogen atoms is also considered in relation to the cooling of the interstellar gas.作者: 鞭打 時間: 2025-3-27 21:15 作者: Memorial 時間: 2025-3-27 23:04 作者: abolish 時間: 2025-3-28 04:26 作者: 公理 時間: 2025-3-28 08:15 作者: 摸索 時間: 2025-3-28 11:00
Optical and IR Emission Lines,To discuss the present understanding of optical and IR emission lines in the interstellar medium, we summarize the basic theory involved, and next see the status of observations and the approximations used to derive the physical parameters.作者: CLAY 時間: 2025-3-28 15:37
Ch. Beal Anderson,L. Ereshefsky. This combination of tests should include culture (with toxin testing of the isolate), demonstration of toxin direct from the faeces and the detection of . antigen. This chapter outlines the methods used to establish the laboratory diagnosis of CDI and also includes the investigation of environment作者: 恃強凌弱的人 時間: 2025-3-28 19:20 作者: ineptitude 時間: 2025-3-28 23:48
Cristian Ciurea,Paul Pocatilu,Florin Gheorghe FiliPresents research works in the field of business informatics.Provides original works presented at IE 2022 held in Bucharest, Romania.Serves as a reference for researchers and practitioners in academia
