標題: Titlebook: Kinematics and Dynamics of Diffuse Astrophysical Media; J. E. Dyson,E. B. Carling Book 1994 Springer Science+Business Media Dordrecht 1994 [打印本頁] 作者: fungus 時間: 2025-3-21 16:21
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書目名稱Kinematics and Dynamics of Diffuse Astrophysical Media年度引用學科排名
書目名稱Kinematics and Dynamics of Diffuse Astrophysical Media讀者反饋
書目名稱Kinematics and Dynamics of Diffuse Astrophysical Media讀者反饋學科排名
作者: BRAWL 時間: 2025-3-21 22:50
Parametric determination of the inclination of Keplerian circumstellar discs from spectropolarimetrcircumstellar disc are presented. It is shown that analysis of the scattered line profiles at different wavelengths which, due to Doppler redistribution, sample different disc regions allows the disc inclination to be determined.作者: crescendo 時間: 2025-3-22 03:07
Jets,s. Recent measurements of the proper motions of HH objects show that even those near the source are moving at about the same speed as the jet fluid. This means that they cannot be due to steady shocks in the jet and the only obvious explanation is that the source is varying.作者: Panacea 時間: 2025-3-22 04:45 作者: outrage 時間: 2025-3-22 09:33 作者: backdrop 時間: 2025-3-22 13:32
Cosmical Gas Dynamics, Why Was It So Difficult?,When the invitation for this meeting reached me, I did not hesitate. Of course, I wished to be present when it was Franz Kahn’s turn for the formal move to say goodbye. Like many of us, he will probably sneak in again through the back door and continue working.作者: 把…比做 時間: 2025-3-22 19:44 作者: Obliterate 時間: 2025-3-22 23:03 作者: 暫時休息 時間: 2025-3-23 05:27
Complex Structure Associated with the Wolf-Rayet Star WR147,The Wolf-Rayet star WR147 is known to be bright at X-ray and radio wavelengths (van der Hucht ., 1981, Caillaut ., 1985, Abbot ., 1986).作者: 產(chǎn)生 時間: 2025-3-23 08:46
The Importance of Continuum Radiation for the Stellar Wind Hydrodynamics of Hot Stars,The contribution of bound-free and free-free processes to the outward acceleration of ζPup is studied and is found to be negligible.作者: Nostalgia 時間: 2025-3-23 10:35
A Simulation of a Jet with the Hiccups,We present results of a numerical simulation of a stellar jet from a source with supersonic variations in the outflow velocity. The simulation is compared with both analytical predictions and observations.作者: 強壯 時間: 2025-3-23 16:00
Herbig Ae/Be Stars,s manifested through optical outflows. It is shown that although there are similarities with analogous outflows from lower mass young stars, those from Herbig Ae/Be stars may be more poorly collimated. Jets, however, are found in at least some cases.作者: 種族被根除 時間: 2025-3-23 21:31 作者: Offset 時間: 2025-3-24 01:52
3-D radiative line transfer for Be star envelopes,ines with blue-shifted central depressions are in contradiction with the observed line shapes. It is concluded that isotropic stationary outflows are not suitable to explain observed asymmetric emission line profiles of Be stars.作者: 高調(diào) 時間: 2025-3-24 05:37 作者: chance 時間: 2025-3-24 08:56
Shaping Planetary Nebulae,n equatorial waistband. The physics of the ensuing evolution seems to be explained nicely by a combination of hydrodynamics coupled with time-dependent stellar ionization and energy loss through nebular radiation. Recent radiation gas dynamic calculations are shown to yield excellent agreement with data.作者: 俗艷 時間: 2025-3-24 12:53
Investigating the Kinematics of the Faint, Giant Haloes of Planetary Nebulae, thin, radially expanding, spherical shell and that of NGC 6826 is more probably a filled spherical shell. The halo of NGC 6720 contains inner and outer shells, the split profiles from the inner halo show that this part of the halo is bipolar in nature.作者: 行乞 時間: 2025-3-24 18:09 作者: Insatiable 時間: 2025-3-24 19:26
Spectroscopic constraints on outflows from BN-type objects,other a more slowly moving optically-thin volume of gas that may, in the case of S106IR at least, be caused by mass loading of the stellar wind. This decomposition is shown to resolve a long-standing problem regarding the relative widths of high and low opacity lines.作者: 要塞 時間: 2025-3-25 02:52 作者: Synchronism 時間: 2025-3-25 03:47
Observational Evidence for Global Oscillations in Be Star Disks,. variations observed in some Be stars are two aspects of the same phenomenon, one-armed global oscillations in a Keplerian disk. We present model profiles and a line fit to support this hypothesis and find good overall agreement.作者: LIMN 時間: 2025-3-25 10:57
Coupled Stellar Jet/Molecular Outflow Models,outflows are identified with the turbulent mixing layer at the edge of a jet, with a turbulent envelope (driven by a large number of internal working surfaces in the jet) and with the wake of one working surface.作者: COST 時間: 2025-3-25 12:06 作者: FILLY 時間: 2025-3-25 19:30 作者: BLOT 時間: 2025-3-26 00:01
Book 1994t in fact this long association and the actual year of the Conference are connected. In 1951 Franz Kahn joined the Astronomy Department at Manchester University and immediately the study of diffuse media, particularly the hydrody- namic aspects, commenced and has flourished ever since. Franz became 作者: 文藝 時間: 2025-3-26 02:08
erence. But in fact this long association and the actual year of the Conference are connected. In 1951 Franz Kahn joined the Astronomy Department at Manchester University and immediately the study of diffuse media, particularly the hydrody- namic aspects, commenced and has flourished ever since. Franz became 978-94-010-4399-1978-94-011-0926-0作者: nauseate 時間: 2025-3-26 06:55
S. M. Scarrott,R. M. J. Scarrott,R. D. Wolstencroft作者: 屈尊 時間: 2025-3-26 11:43
A. F. J. Moffat,S. Lépine,R. N. Henriksen,C. Robert作者: 連接 時間: 2025-3-26 13:49
Kinematics and Dynamics of Diffuse Astrophysical Media作者: 小步走路 時間: 2025-3-26 19:11
Kinematics and Dynamics of Diffuse Astrophysical Media978-94-011-0926-0作者: Adornment 時間: 2025-3-26 23:27
Shaping Planetary Nebulae,ssful models are two-dimensional interacting stellar wind models for which the PN nucleus is assumed to originally expel much or most of its mass in an equatorial waistband. The physics of the ensuing evolution seems to be explained nicely by a combination of hydrodynamics coupled with time-dependen作者: LANCE 時間: 2025-3-27 02:39 作者: Blood-Clot 時間: 2025-3-27 05:36
Shock Modelling of Planetary Nebulae,y our analysis to the Planetary Nebulae NGC 6905 and NGC 6537. A detailed spectroscopic study of these objects reveals the existence of high nuclear velocities, together with complex kinematic structures and unusual emission line intensities. Shock ionization clearly plays a key role in these nebula作者: 值得贊賞 時間: 2025-3-27 11:09 作者: 一小塊 時間: 2025-3-27 14:24
First Wavelet Analysis of Emission Line Variations in Wolf-Rayet Stars, powerful, objective technique of wavelet analysis. Results for the substructures in one WR star so far show that the scaling laws between (a) flux and velocity dispersion and (b) lifetime and flux, combined with (c) their mass spectrum, strongly support the hypothesis that we are seeing the high ma作者: 烤架 時間: 2025-3-27 19:29
Herbig Ae/Be Stars,m. After a historical introduction, we briefly review their optical and UV spectroscopic properties. We consider the evidence for and against disks around Herbig Ae/Be stars; the existence of which remains highly controversial. We also examine in-depth their interaction with the surrounding medium a作者: Fulminate 時間: 2025-3-27 21:58 作者: 盡管 時間: 2025-3-28 02:26
Radiatively Driven Winds Using Lagrangian Hydrodynamics,can only be applied to simple geometries. Presented here are preliminary results of a particle based Lagrangian code (applied to a simple 1D radiatively driven wind test case), which will be able to resolve structure down to the smallest scales without becoming temporally prohibitive. This approach 作者: Encephalitis 時間: 2025-3-28 09:33
Parametric determination of the inclination of Keplerian circumstellar discs from spectropolarimetrcircumstellar disc are presented. It is shown that analysis of the scattered line profiles at different wavelengths which, due to Doppler redistribution, sample different disc regions allows the disc inclination to be determined.作者: 預示 時間: 2025-3-28 14:05 作者: 貴族 時間: 2025-3-28 16:06 作者: 主動脈 時間: 2025-3-28 20:59 作者: Exonerate 時間: 2025-3-29 01:21
Jets,s. Recent measurements of the proper motions of HH objects show that even those near the source are moving at about the same speed as the jet fluid. This means that they cannot be due to steady shocks in the jet and the only obvious explanation is that the source is varying.作者: 手術刀 時間: 2025-3-29 04:06 作者: 起來了 時間: 2025-3-29 07:35 作者: 贊美者 時間: 2025-3-29 15:04 作者: DEMUR 時間: 2025-3-29 17:26 作者: FOVEA 時間: 2025-3-29 21:26 作者: 藐視 時間: 2025-3-30 02:57
Honest Signals and Their Contribution to the Automatic Analysis of Personality Traits – A Comparativs of Control. In particular, we investigate the predictive power of four classes of speech honest signal features (Conversational Activity, Emphasis, Influence, and Mimicry), along with three fidgeting visual features by systematically comparing the results obtained by classifiers using them.作者: 緯度 時間: 2025-3-30 05:24 作者: prosthesis 時間: 2025-3-30 10:36
Improved Genome Editing via Oviductal Nucleic Acids Delivery (,GONAD): Protocol Steps and Additional Notes,ly and rapidly than before. In most cases, GE mice are produced by microinjection (MI) or by in vitro electroporation (EP) of CRISPR reagents into fertilized eggs (zygotes). Both of these approaches require ex vivo handling of isolated embryos and their subsequent transfer into another set of mice (作者: PET-scan 時間: 2025-3-30 12:59 作者: NUL 時間: 2025-3-30 20:07
Michal Bassani-Sternbergver, only indirect markers for apoptosis, such as soluble FAS, can be measured in plasma. During the later stages of apoptosis, nucleosomes are released from cell’s chromatin by internucleosomal cleavage by endonucleases. We investigated whether circulating nucleosomes constitute a marker for apoptosis in sepsis.作者: 石墨 時間: 2025-3-30 22:01
An Abstract Machine for the Old Value Retrievalcalled here sufficiently persistent, as opposed to persistent and partially persistent structures. A space-bound on the structure size is given. It is also demonstrated that methods which do not have post-conditions can be abstracted away.作者: 不能根除 時間: 2025-3-31 01:23 作者: appall 時間: 2025-3-31 06:31
Saurabh Daripa,Amrish K. Panwarore packaging to avoid any contamination. Along with the evidence found, control samples of the same must be collected using the same protocol simultaneously for the purpose of analysis and comparison in the laboratory. The initials of the officer and the date should be mentioned accurately. An evid作者: laxative 時間: 2025-3-31 09:31
Abstraction for Falsificationction for verification may be too restrictive when used for falsification, and that a new framework is needed in order to take advantage of the weaker definition of soundness in the falsification setting..We present such a framework, show that it is indeed stronger (than other abstraction frameworks作者: Collar 時間: 2025-3-31 15:47 作者: indifferent 時間: 2025-3-31 19:13 作者: Kindle 時間: 2025-3-31 23:38 作者: 蕨類 時間: 2025-4-1 03:55
RSA Weak Public Keys Available on the Internette to. We show that the percentage of broken keys with 512 bits is 3.7?%, while the percentage of broken keys with 1024 bits is 0.05?%. The smaller value is due to the fact that factorization of large numbers includes new prime numbers, unused in the small keys.
