標(biāo)題: Titlebook: Astrophysics of the Interstellar Medium; Giovanni Carraro Textbook 2021 The Editor(s) (if applicable) and The Author(s), under exclusive l [打印本頁] 作者: 存貨清單 時(shí)間: 2025-3-21 19:24
書目名稱Astrophysics of the Interstellar Medium影響因子(影響力)
書目名稱Astrophysics of the Interstellar Medium影響因子(影響力)學(xué)科排名
書目名稱Astrophysics of the Interstellar Medium網(wǎng)絡(luò)公開度
書目名稱Astrophysics of the Interstellar Medium網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Astrophysics of the Interstellar Medium被引頻次
書目名稱Astrophysics of the Interstellar Medium被引頻次學(xué)科排名
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書目名稱Astrophysics of the Interstellar Medium年度引用學(xué)科排名
書目名稱Astrophysics of the Interstellar Medium讀者反饋
書目名稱Astrophysics of the Interstellar Medium讀者反饋學(xué)科排名
作者: 斑駁 時(shí)間: 2025-3-21 23:24
Foundation Mathematics for Engineersnes of force. The pressure is balanced by the pressure of the surrounding regions and what remains is the tension along the induction lines which acts to bring them back to the equilibrium position through a series of oscillations.作者: Adulterate 時(shí)間: 2025-3-22 00:29
Knowledge Acquired by Foundation Models,e of the star generates the emission. The detailed shape of the profile depends on the geometry of the envelope, the velocity trend, the density and the nature of the absorption and emission processes.作者: condescend 時(shí)間: 2025-3-22 06:06 作者: 混亂生活 時(shí)間: 2025-3-22 10:22 作者: coagulate 時(shí)間: 2025-3-22 13:42 作者: murmur 時(shí)間: 2025-3-22 17:41
Textbook 2021a University.?.From the cold molecular phase in which stars and planetary systems form, to the very hot coronal gas that surrounds galaxies and galaxy clusters, the ISM is everywhere. Studying its properties is vital for the exploration of virtually any field in astronomy and cosmology. These notes 作者: Osteons 時(shí)間: 2025-3-22 23:17
2198-7882 erives all of its formulas from first principles.Features exThis book is based on a series of lectures for an Astrophysics of the Interstellar Medium (ISM) master’s degree in Astrophysics and Cosmology at Padova University.?.From the cold molecular phase in which stars and planetary systems form, to作者: savage 時(shí)間: 2025-3-23 05:23
https://doi.org/10.1007/978-3-030-91963-4ances made with photometry, a distance that was overestimated precisely for the absorbing action of solid dust particles. The study of the spatial distribution of these led to the conclusion that dust was associated with the interstellar gas.作者: Endoscope 時(shí)間: 2025-3-23 08:44 作者: Venules 時(shí)間: 2025-3-23 13:04 作者: 豐滿中國 時(shí)間: 2025-3-23 17:44 作者: Airtight 時(shí)間: 2025-3-23 20:37 作者: 故意 時(shí)間: 2025-3-24 01:41
Creating a User Registration Database, low-mass and large-mass stars are observed. More in detail, considering the “cores”, i.e. the densest regions of molecular clouds with . cm., we can define a subdivision of the “cores” into two categories:作者: palpitate 時(shí)間: 2025-3-24 04:00 作者: 翻布尋找 時(shí)間: 2025-3-24 07:42 作者: Lamina 時(shí)間: 2025-3-24 11:13
Textbook 2021s switched on and its role in modulating shock waves and contrasting gravity is studied. Part Three describes dust and its properties, followed by the main stellar sources of energy. The last two chapters respectively address the various components of the ISM and molecular clouds and star formation.作者: TRAWL 時(shí)間: 2025-3-24 17:36
2198-7882 art Three describes dust and its properties, followed by the main stellar sources of energy. The last two chapters respectively address the various components of the ISM and molecular clouds and star formation.978-3-030-75295-8978-3-030-75293-4Series ISSN 2198-7882 Series E-ISSN 2198-7890 作者: 微生物 時(shí)間: 2025-3-24 21:26
Fundamental Equations for Ideal Fluids,l agitation. Let us analyze the dependence of such forces on intermolecular distance, as illustrated in Fig.?.. Forces are repulsive when ., attractive when . and in an equilibrium configuration when ..作者: 地名表 時(shí)間: 2025-3-25 00:26
Acoustic Waves,s) the surrounding medium; if its motion is slow the air slides along it but, if the speed is high, air gets compressed and the pressure variation generates oscillations propagating around it in the form of a wave. One would argue that as a consequence of this molecules simply move from denser to le作者: growth-factor 時(shí)間: 2025-3-25 06:24
Real Fluids, temperature, chemical composition, etc.). If any of these quantities is not uniformly distributed, the system is not in equilibrium and exchanges occur of a mechanical or thermal nature between nearby elements until equilibrium is eventually achieved.作者: Cardioplegia 時(shí)間: 2025-3-25 08:11
The Interstellar Medium,l conductivity there is no thermal contact with the surrounding medium and the dissipation of energy by viscosity is negligible. In general, viscosity and thermal conduction are also of little importance in interstellar gas. Consider the role of thermal conduction in a molecular cloud of size ., wit作者: fidelity 時(shí)間: 2025-3-25 14:44
Electrodynamics and Magnetohydrodynamics, electrons and on the ions producing currents. In turn currents cause alterations in the electro-magnetic field: hence, we have to do with a complicated coupled system of matter and fields. We focus on conductor fluids, that is, on ionised gases. The fundamental difference between a non-conducting g作者: 萬靈丹 時(shí)間: 2025-3-25 18:07
Magnetohydrodynamic Waves, the magnetic tension tends to bring them back into rectilinear form, however causing transverse oscillations. This type of magnetohydrodynamic wave, called Alfven wave, is the only one possible in an incompressible fluid. If we assume infinite electrical conductivity, the magnetic lines of force ar作者: 打折 時(shí)間: 2025-3-25 21:47 作者: 上下倒置 時(shí)間: 2025-3-26 00:46
Stellar Winds, is called stellar wind. The existence of these winds was revealed mostly through the UV spectra obtained with the IUE satellite; the resonance lines of these spectra have P-Cygni profiles (see Fig.?.). These profiles consist of an absorption component shifted to shorter wavelengths, and an emission作者: Oration 時(shí)間: 2025-3-26 04:26 作者: 含鐵 時(shí)間: 2025-3-26 11:42
Star Formation,of formation of the two types of stars are spatially separated, more precisely there are regions where only low-mass stars are formed and regions where both low-mass and massive stars are formed. For example, the Taurus region does not seem to contain stars more massive than 2 ., while in Orion both作者: ectropion 時(shí)間: 2025-3-26 14:27
https://doi.org/10.1007/978-3-030-75293-4Interstellar Medium Graduate Textbook; Astrophysics Textbook; Magneto Hydro Dynamics; Turbolence; Inters作者: 在前面 時(shí)間: 2025-3-26 19:05 作者: Matrimony 時(shí)間: 2025-3-27 00:59 作者: 搜集 時(shí)間: 2025-3-27 01:59
Foundation Mac OS X Web Developmentl agitation. Let us analyze the dependence of such forces on intermolecular distance, as illustrated in Fig.?.. Forces are repulsive when ., attractive when . and in an equilibrium configuration when ..作者: 搖曳的微光 時(shí)間: 2025-3-27 08:58
Foundation Mathematics for Computer Science temperature, chemical composition, etc.). If any of these quantities is not uniformly distributed, the system is not in equilibrium and exchanges occur of a mechanical or thermal nature between nearby elements until equilibrium is eventually achieved.作者: tinnitus 時(shí)間: 2025-3-27 11:23
Foundation Mathematics for Computer Sciencel conductivity there is no thermal contact with the surrounding medium and the dissipation of energy by viscosity is negligible. In general, viscosity and thermal conduction are also of little importance in interstellar gas. Consider the role of thermal conduction in a molecular cloud of size ., with temperature . and density ..作者: 減去 時(shí)間: 2025-3-27 14:09 作者: misanthrope 時(shí)間: 2025-3-27 21:46 作者: 討好美人 時(shí)間: 2025-3-27 23:18 作者: 易怒 時(shí)間: 2025-3-28 02:20 作者: 過分自信 時(shí)間: 2025-3-28 07:53
Foundation Mathematics for Computer Science electrons and on the ions producing currents. In turn currents cause alterations in the electro-magnetic field: hence, we have to do with a complicated coupled system of matter and fields. We focus on conductor fluids, that is, on ionised gases. The fundamental difference between a non-conducting g作者: 暫時(shí)過來 時(shí)間: 2025-3-28 12:21
Foundation Mathematics for Engineers the magnetic tension tends to bring them back into rectilinear form, however causing transverse oscillations. This type of magnetohydrodynamic wave, called Alfven wave, is the only one possible in an incompressible fluid. If we assume infinite electrical conductivity, the magnetic lines of force ar作者: abduction 時(shí)間: 2025-3-28 17:52
https://doi.org/10.1007/978-3-030-91963-4orly convincing result: their diameters were an increasing function of distance. The origin of this result was linked to the determination of the distances made with photometry, a distance that was overestimated precisely for the absorbing action of solid dust particles. The study of the spatial dis作者: AXIOM 時(shí)間: 2025-3-28 19:25 作者: Entrancing 時(shí)間: 2025-3-29 01:39
Creating a User Registration Database,arefied medium. This theory is based on the hypothesis of a stationary state in dynamic and thermal equilibrium, the fundamental principles of which have been set out in Sect.?.. In the light of the thermal stability analysis, the functional dependence of the cooling rate on the temperature is able 作者: conjunctivitis 時(shí)間: 2025-3-29 03:54 作者: 最小 時(shí)間: 2025-3-29 10:25
Foundation Mathematics for Computer ScienceThe speed of sound is a critical speed (remember what was said in Sect.?. about the time required to restore dynamic equilibrium). In relation to . the fluid motions are classified into subsonic (.) and supersonic (.). We use to introduce the Mach number ., so the motions will be subsonic or supersonic depending on whether . or ..作者: erythema 時(shí)間: 2025-3-29 15:04
https://doi.org/10.1007/978-3-319-21437-5Werner Heisenberg once said: “When I meet God, I am going to ask him two questions: Why relativity? And why turbulence? I really believe he will have an answer for the first.”作者: 顯而易見 時(shí)間: 2025-3-29 17:49 作者: 細(xì)頸瓶 時(shí)間: 2025-3-29 19:49 作者: FER 時(shí)間: 2025-3-30 01:04 作者: 貞潔 時(shí)間: 2025-3-30 06:31 作者: caldron 時(shí)間: 2025-3-30 11:18 作者: HOWL 時(shí)間: 2025-3-30 12:49 作者: 泥沼 時(shí)間: 2025-3-30 19:33
Motion of a Plasma in a Magnetic Field,The magnetic stress tensor is defined by: 作者: 疾馳 時(shí)間: 2025-3-30 23:44 作者: curriculum 時(shí)間: 2025-3-31 04:42 作者: acrophobia 時(shí)間: 2025-3-31 05:31
Molecular Clouds,Molecular clouds are the densest and coldest component of the ISM. They are made of H in its molecular form (.), and by many other molecules, although much less abundant than H. Hundreds of species have recently been detected by ALMA in the sub-millimeter regime, where most molecules show rotational emission lines.作者: 責(zé)問 時(shí)間: 2025-3-31 11:34 作者: ABHOR 時(shí)間: 2025-3-31 13:38 作者: MUT 時(shí)間: 2025-3-31 18:04
Fundamental Equations for Ideal Fluids,l agitation. Let us analyze the dependence of such forces on intermolecular distance, as illustrated in Fig.?.. Forces are repulsive when ., attractive when . and in an equilibrium configuration when ..作者: AWL 時(shí)間: 2025-3-31 23:44
