標(biāo)題: Titlebook: Magnetic Fields and Star Formation; Theory Versus Observ A. I. Gómez Castro,M. Heyer,R. E. Pudritz Book 2004 Springer Science+Business Medi [打印本頁] 作者: 變成小松鼠 時(shí)間: 2025-3-21 18:29
書目名稱Magnetic Fields and Star Formation影響因子(影響力)
書目名稱Magnetic Fields and Star Formation影響因子(影響力)學(xué)科排名
書目名稱Magnetic Fields and Star Formation網(wǎng)絡(luò)公開度
書目名稱Magnetic Fields and Star Formation網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Magnetic Fields and Star Formation被引頻次
書目名稱Magnetic Fields and Star Formation被引頻次學(xué)科排名
書目名稱Magnetic Fields and Star Formation年度引用
書目名稱Magnetic Fields and Star Formation年度引用學(xué)科排名
書目名稱Magnetic Fields and Star Formation讀者反饋
書目名稱Magnetic Fields and Star Formation讀者反饋學(xué)科排名
作者: entrance 時(shí)間: 2025-3-21 23:14
Turbulence in the Star-Forming Interstellar Medium: Steps Toward Constraining Theories with Observat a rapid pace, aided in part by numerical simulations. These increased capabilities on both fronts open new opportunities for strengthening the links between observation and theory, and for meaningful comparisons between the two.作者: Trigger-Point 時(shí)間: 2025-3-22 04:15
The Tiny-Scale Atomic Structure: Gas Cloudlets or Scintillation Phenomenon ?ns of B0823+26 and B1133+16 are similar on scales of 10–20, 350 and 500 AU. The large number of non detections of the tiny scale atomic structure suggests that the AU-sized structure is not ubiquitous in the interstellar medium.作者: 繁殖 時(shí)間: 2025-3-22 05:21 作者: insecticide 時(shí)間: 2025-3-22 12:09 作者: Axon895 時(shí)間: 2025-3-22 15:27 作者: Console 時(shí)間: 2025-3-22 19:08
Magnetic Flux Transport in the ISM through Turbulent Ambipolar Diffusionether turbulence can enhance the ambipolar diffusion rate sufficiently to explain the observed weak correlations. The numerical method is based on a gas-kinetic scheme with very low numerical diffusivity, thus allowing us to separate numerical and physical diffusion effects.作者: conjunctiva 時(shí)間: 2025-3-22 22:42 作者: 討好美人 時(shí)間: 2025-3-23 04:54 作者: 注視 時(shí)間: 2025-3-23 09:10 作者: Anticoagulants 時(shí)間: 2025-3-23 13:31 作者: 收養(yǎng) 時(shí)間: 2025-3-23 14:32
Scaling Relations of Supersonic Turbulence in Molecular Cloudsis highly intermittent; we describe its statistical properties by obtaining scaling of velocity-difference structure functions. This scaling was analytically predicted in Boldyrev (2002), confirmed in numerical simulations by Boldyrev et al. (2002), and discovered in observations by Padoan et al. (2003).作者: ZEST 時(shí)間: 2025-3-23 20:50 作者: jagged 時(shí)間: 2025-3-23 22:34
Structure of Molecular Cloudsnnection with the diffuse medium, their multi-fractal characteristics and the diversity of their small-scale structure, where cold and dense gas may coexist with dilute and warm gas. Stuctures of essentially pure velocity origin are uncovered and seen as a possible signature of the intermittency of turbulence dissipation.作者: 舉止粗野的人 時(shí)間: 2025-3-24 02:36
http://image.papertrans.cn/m/image/621226.jpg作者: GEM 時(shí)間: 2025-3-24 08:13 作者: FOLLY 時(shí)間: 2025-3-24 10:41 作者: ARCH 時(shí)間: 2025-3-24 17:11 作者: fatty-streak 時(shí)間: 2025-3-24 22:34 作者: Monocle 時(shí)間: 2025-3-25 01:53
High-Resolution Simulations of Nonhelical MHD Turbulencere function exponent that is found to be .. = 0.70, suggesting a .. spectrum. The third-order structure function scaling exponent is very close to unity,—in agreement with Goldreich—Sridhar theory..Adding an imposed field tends to suppress the small-scale magnetic field. We find that at large scales作者: 雪白 時(shí)間: 2025-3-25 05:46 作者: MAUVE 時(shí)間: 2025-3-25 09:14
MHD Simulations of the ISM: The Importance of the Galactic Magnetic Field on the ISM “Phases”the mass in the disk is concentrated in the thermally unstable regime 10. < T ≤ 10. K with ~30% of the disk mass enclosed in the T ≤ 10. K gas. The hot gas in contrast is controlled by the thermal pressure, since magnetic field lines are swept towards the dense compressed walls.作者: Density 時(shí)間: 2025-3-25 13:40
Book 2004 this intensive week of work. The book is written in a comprehensive manner and reviews our current knowledge of the subject. It also represents an updated account of the ideas and thoughts of the scientists working in the field of Star Formation. The contributions are presented in six chapters whic作者: Exclude 時(shí)間: 2025-3-25 18:06 作者: Arbitrary 時(shí)間: 2025-3-25 22:02 作者: 分解 時(shí)間: 2025-3-26 00:38 作者: CHAFE 時(shí)間: 2025-3-26 05:20 作者: 冒失 時(shí)間: 2025-3-26 12:03
A. Lazarian,J. Cho on chronic wounds. The range of topical agents in use at this time will range from matrix metalloproteinases inhibitors, anti-TNF alpha drugs, and nonsteroidal anti-inflammatory agents. Careful evaluation of wound bed and sometimes pathological assessment with a biopsy are mandatory before starting作者: BINGE 時(shí)間: 2025-3-26 15:57 作者: 不近人情 時(shí)間: 2025-3-26 19:04
Fabian Heitsch,Ellen G. Zweibel,Adrianne D. Slyz,Julien E. G. Devriendt作者: 清醒 時(shí)間: 2025-3-26 23:44
Georgi Pavlovski,Michael D. Smith,Mordecai-Mark Mac Low,Alexander Rosen作者: Outmoded 時(shí)間: 2025-3-27 04:48
Edith Falgarone,Pierre Hily-Blant,Fran?ois Levrier作者: 大氣層 時(shí)間: 2025-3-27 08:49 作者: 使乳化 時(shí)間: 2025-3-27 11:03 作者: Alpha-Cells 時(shí)間: 2025-3-27 16:15
Martin Houde,Ruisheng Peng,Hiroshige Yoshida,Roger H. Hildebrand,Thomas G. Phillips,C. Darren Dowell作者: 長矛 時(shí)間: 2025-3-27 19:49 作者: folliculitis 時(shí)間: 2025-3-28 01:53
Basic Properties of Compressible MHD Turbulence: Implications for Molecular Cloudslly accepted concepts. First, the MHD turbulence is not so messy as it is usually believed. In fact, the notion of strong nonlinear coupling of compressible and incompressible motions is not tenable. Alfven, slow and fast modes of MHD turbulence follow their own cascades and exhibit degrees of aniso作者: OVER 時(shí)間: 2025-3-28 05:19 作者: Picks-Disease 時(shí)間: 2025-3-28 06:30 作者: Conducive 時(shí)間: 2025-3-28 10:55 作者: aggressor 時(shí)間: 2025-3-28 16:57
Hydrodynamical Simulations of Molecular Dynamics in Supersonic Turbulent Flowappropriate chemical processes. We investigate regimes of decaying high-speed molecular turbulence. Here we analyse PDFs of density for the volume, mass, molecular mass and the energy distribution over the range of scales. We compare our results to those previously obtained for isothermal turbulence作者: 發(fā)怨言 時(shí)間: 2025-3-28 21:04
Observational Magnetogasdynamics: 21 Years of HI Zeeman Splitting Measurements...and Moreewhat more WNM than CNM, and at least half of the WNM is not thermally stable. The CNM has typical turbulent Mach number 3. Magnetic fields in the CNM are not as large as expected from the classical flux-freezing argument; neither are magnetic fields always strong enough for the Alfven velocity to e作者: inflate 時(shí)間: 2025-3-28 23:37
Structure of Molecular Cloudsnnection with the diffuse medium, their multi-fractal characteristics and the diversity of their small-scale structure, where cold and dense gas may coexist with dilute and warm gas. Stuctures of essentially pure velocity origin are uncovered and seen as a possible signature of the intermittency of 作者: Engaging 時(shí)間: 2025-3-29 04:56
The Tiny-Scale Atomic Structure: Gas Cloudlets or Scintillation Phenomenon ?nd significant variations in optical depth profiles over periods of 4 months and 9 years. The upper limits on the optical depth variations in directions of B0823+26 and B1133+16 are similar on scales of 10–20, 350 and 500 AU. The large number of non detections of the tiny scale atomic structure sugg作者: pancreas 時(shí)間: 2025-3-29 08:47 作者: WAIL 時(shí)間: 2025-3-29 13:34
BIMA and JCMT Spectropolarimetric Observations of the CO J = 2 ? 1 Line Towards Orion KL/IRc2ation fraction of the JCMT CO . = 2 ? 1 spectra presents a clear decrease towards the center of the line, as expected, due to the increase of the optical depth. The position angle remains constant along the spectral line, except at the line center, where the highest optical depth and lower fractiona作者: temperate 時(shí)間: 2025-3-29 19:02 作者: 矛盾心理 時(shí)間: 2025-3-29 22:27
Fragmentation and Structure Formationn of one level into the next, with the formation of stars as its last step. Within this framework, I then give an overview of the contributions to this session. Numerical work addresses, at the largest scales, the shaping and formation of structures in the ISM through turbulence driven by stellar en作者: Chandelier 時(shí)間: 2025-3-30 01:17
Turbulent Fragmentation and Star Formationing relationships, the “quiescent” (subsonic) nature of many star-forming cores, their energy balance, their synthesized polarized dust emission, the ages of stars associated with the molecular gas from which they have formed, the mass spectra of clumps, and the density and column density probabilit作者: Fracture 時(shí)間: 2025-3-30 07:19 作者: 串通 時(shí)間: 2025-3-30 10:01 作者: GENUS 時(shí)間: 2025-3-30 14:08
are responsibilities. The book studies the complex combination of and the relationships between local political processes, policies, institutions, structural conditions and outputs, as well as outcomes for the women’s labour market integration. It demonstrates how cultural settings and multi-level g作者: monopoly 時(shí)間: 2025-3-30 18:33 作者: 開頭 時(shí)間: 2025-3-31 00:22 作者: 花爭吵 時(shí)間: 2025-3-31 04:13
Benjamin D. G. Chandransystems and the territorial organization of social services.This book discusses local area planning in the Lombardy region of Italy. The book provides valuable insights about the development of local welfare systems and the territorial organization of social services through the analysis of the evol作者: 含糊 時(shí)間: 2025-3-31 08:43
A. Lazarian,J. Choapeutic strategies..The goal of caregiver should be to better understand when there is a necessity to provide the wound bed and surrounding skin with an anti-inflammatory therapy. The role of exudate on this matter is fundamental and more and more information have been provided to characterize the v
