標(biāo)題: Titlebook: Jets in Young Stellar Objects; Theory and Observati A. J. L. Fernandes,P. J. V. Garcia,J. J. G. Lima Book 2003 Springer Science+Business Me [打印本頁] 作者: Croching 時(shí)間: 2025-3-21 19:47
書目名稱Jets in Young Stellar Objects影響因子(影響力)
書目名稱Jets in Young Stellar Objects影響因子(影響力)學(xué)科排名
書目名稱Jets in Young Stellar Objects網(wǎng)絡(luò)公開度
書目名稱Jets in Young Stellar Objects網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Jets in Young Stellar Objects被引頻次
書目名稱Jets in Young Stellar Objects被引頻次學(xué)科排名
書目名稱Jets in Young Stellar Objects年度引用
書目名稱Jets in Young Stellar Objects年度引用學(xué)科排名
書目名稱Jets in Young Stellar Objects讀者反饋
書目名稱Jets in Young Stellar Objects讀者反饋學(xué)科排名
作者: Demonstrate 時(shí)間: 2025-3-21 23:01 作者: 刪除 時(shí)間: 2025-3-22 02:34
The Structure of Young Stellar Jets and Winds Revealed By High Resolution [Fe Ii] λL.644μM Line Obsediagrams of the [Fe II] λ 1.644 μm emission line revealed remarkably similar characteristics for the two sources, showing two distinct velocity components separated from each other in both velocity and space with the entire emission range blueshifted with respect to the stellar velocity. The high ve作者: 搜集 時(shí)間: 2025-3-22 06:29
Star-Driven Wind and Jet Models-wind models. We emphazise the roles of the magnetic rotator and the disk in the formation and the evolution of the jet. We conjecture that with time both the efficiency of the magnetic rotator and the role of the disk as a primary source for the wind decline.作者: SLUMP 時(shí)間: 2025-3-22 11:05 作者: Kidney-Failure 時(shí)間: 2025-3-22 16:38
New Ideas on Jets and Outflows Interactionsng the jet, the molecular outflow is powered by the infailing matter and follows a circulation pattern around the central object without necessarily being entrained by the jet. The model produces a heated pressure-driven outflow with magneto-centrifugal acceleration and collimation. We will try to c作者: Evolve 時(shí)間: 2025-3-22 19:06
Continuum Excess Emission in Young Low Mass Stars understanding about the CTTS systems impinges directly on our ability to achieve a deeper knowledge of the final stages of low mass stars formation, of the pre-main sequence history of the Sun and even on the processes that lead to planet formation. Here I present a portion of the . of the CTTS sys作者: Dendritic-Cells 時(shí)間: 2025-3-23 00:35 作者: 昏暗 時(shí)間: 2025-3-23 03:24 作者: 縮短 時(shí)間: 2025-3-23 06:06 作者: 名字 時(shí)間: 2025-3-23 11:53 作者: 手術(shù)刀 時(shí)間: 2025-3-23 14:47
2- and 3-D Simulations of Magnetocentrifugal Disk-Winds: Acceleration and Stabilityct launching conditions on the disk, such as the distributions of magnetic flux and mass ejection rate, are poorly known. They could be constrained from observations at large distances, provided that a robust model is available to link the observable properties of the jets and winds at the large dis作者: Facet-Joints 時(shí)間: 2025-3-23 21:25
Hh 111 Stis Observations and Their Analysis Using Analytical and Numerical Modelsupersonic proper motions. These structures, we believe, are the result of a variable ejection from the source, which leads to the formation of . or small bowshock within the jet beam. In this paper we present a long-slit spectrum of Herbig-Haro object HH 111 obtained with STIS and an interpretation 作者: conceal 時(shí)間: 2025-3-24 01:35 作者: Bravura 時(shí)間: 2025-3-24 02:36
Three-Dimensional Simulations of Jets From Keplerian Disks: Stability Issues. We investigate the outflow that arises from a magnetized accretion disk that is initially in hydrostatic balance with its surrounding cold corona. Our simulations show that jets maintain their long-term stability through a self-limiting process wherein the average Alfvénic Mach number within the j作者: alabaster 時(shí)間: 2025-3-24 07:04
Mhd Simulations of Jets From Accretion Disksly. Although it was considered that this kind of simulations only shows the transient phenomena of jets, we found that the outflow and accretion flow reached a quasi-steady state by performing a long-term calculation in a large calculation region. Though the final stage is not exactly the steady sta作者: VOC 時(shí)間: 2025-3-24 10:47 作者: Transfusion 時(shí)間: 2025-3-24 18:48 作者: 惰性氣體 時(shí)間: 2025-3-24 19:25 作者: MAIZE 時(shí)間: 2025-3-24 23:35 作者: PON 時(shí)間: 2025-3-25 03:38
Daniel F.M. Folhanducting experiments, it is important to be mindful of what scale to sample at; the “correct” scale depends on the research question and the organism(s) of interest. Frequently, patterns seen at one scale will be different – even opposite – at another scale, which introduces difficulties with extrap作者: 排名真古怪 時(shí)間: 2025-3-25 07:57
Suzan Edwardst tools and techniques than what researchers working in terrestrial landscapes use. I illustrate how landscape ecologists can learn from collaborations with marine biologists, aquatic, behavioural and acoustic ecologists to develop experimental approaches that address questions about space use in th作者: 雪白 時(shí)間: 2025-3-25 13:31 作者: largesse 時(shí)間: 2025-3-25 18:35
http://image.papertrans.cn/j/image/500886.jpg作者: Digitalis 時(shí)間: 2025-3-25 23:05
Star-Driven Wind and Jet Models-wind models. We emphazise the roles of the magnetic rotator and the disk in the formation and the evolution of the jet. We conjecture that with time both the efficiency of the magnetic rotator and the role of the disk as a primary source for the wind decline.作者: 強(qiáng)制性 時(shí)間: 2025-3-26 03:43
Continuum Excess Emission in Young Low Mass Stars understanding about the CTTS systems impinges directly on our ability to achieve a deeper knowledge of the final stages of low mass stars formation, of the pre-main sequence history of the Sun and even on the processes that lead to planet formation. Here I present a portion of the . of the CTTS systems and some . in this field.作者: 歡呼 時(shí)間: 2025-3-26 05:43 作者: Coronary-Spasm 時(shí)間: 2025-3-26 11:08 作者: 跳動(dòng) 時(shí)間: 2025-3-26 14:41 作者: altruism 時(shí)間: 2025-3-26 19:07
A.I. GóMez De Castro,C. Ferro-FontáNst for the audience, in which interpretation and meaning are forever suspended in the act of revision; a play in which the question of what and who has been represented is elusive. Instead of giving his audience a ‘retrospect’ of his life, Krapp is forever ‘embarking’ on a new retrospect. It is, per作者: conservative 時(shí)間: 2025-3-26 23:26
Thibaut Lery of fourteen years exists in their proposed tradition from the death of Yeats in 1939 to the premiere of Beckett’s En . in 1953. It follows that the plays of this period have been written out of a reading of a linear chronological tradition of modern Irish drama. This study examines the experimental作者: 有害 時(shí)間: 2025-3-27 03:41 作者: 有助于 時(shí)間: 2025-3-27 09:06
Daniel F.M. Folhaystems with too many variables to model easily but too few to make averaging a meaningful solution. Finally, there is the issue of non-stationarity. Non-stationary processes are those where the means, variance and co-variances change over time – often in unpredictable, stochastic ways. I offer sugge作者: 維持 時(shí)間: 2025-3-27 09:29 作者: 傾聽 時(shí)間: 2025-3-27 15:41 作者: 故意釣到白楊 時(shí)間: 2025-3-27 20:17 作者: 蛛絲 時(shí)間: 2025-3-27 22:33 作者: adroit 時(shí)間: 2025-3-28 05:33
Mhd Simulations of the Long-Term Evolution of a Dipolar Magnetosphere Surrounded By an Accretion Dis 30° to 55° depending on the ratio of the mass flow rates of disk wind and stellar wind. The maximum speed of the outflow is about the Keplerian speed at the inner disk radius. An axial jet forms during the first decades of rotations. However, this feature does not survive on the very long time scal作者: 現(xiàn)代 時(shí)間: 2025-3-28 07:25 作者: AV-node 時(shí)間: 2025-3-28 11:08
Three-Dimensional Simulations of Jets From Keplerian Disks: Stability Issuesf the outflow into the stretched, poloidal field lines of the distorted jet. This too has the effect of increasing the Alfvén speed and thereby reducing the Alfvénic Mach number. The jet is able to survive the onset of the more destructive . = 1 mode in this way.作者: Maximizer 時(shí)間: 2025-3-28 18:07 作者: Respond 時(shí)間: 2025-3-28 21:48 作者: 浪費(fèi)物質(zhì) 時(shí)間: 2025-3-29 00:08
T.A. Gardiner,A. Frank,E.G. Blackman,S.V. Lebedev,J.P. Chittenden,D. Ampleford,S.N. Bland,A. Ciardi,作者: 類型 時(shí)間: 2025-3-29 03:51
K. Tsinganos,N. Vlahakis,S. Bogovalov,C. Sauty,E. Trussoni,J.J.G. Lima作者: 簡潔 時(shí)間: 2025-3-29 09:24
The Structure of Young Stellar Jets and Winds Revealed By High Resolution [Fe Ii] λL.644μM Line Obseinig a broad line width. The HVC is located farther away from the origin and is more extended than the LVC. Our results suggest that the HVC is a well-collimated jet originating from the region close to the star, while the LVC is a widely-opened wind accelerated in the region near the inner edge of the accretion disk.作者: 要素 時(shí)間: 2025-3-29 15:09
Photoionization of Cool Mhd Disk Windstar. However, it is difficult to foresee how temperatures as high as ～ 5 x 10. can be reached unless a significant fraction of the X-rays radiation is produced by magnetic reconnection at the boundary between the stellar magnetosphere and the accretion disk.作者: 值得尊敬 時(shí)間: 2025-3-29 15:43 作者: 推延 時(shí)間: 2025-3-29 21:28
Magnetic Star-Disk Interaction in Classical T Tauri Systemsa solar-mass central star, an accretion rate of 10..⊙/., and a viscosity parameter αss = 0.01, a field strength of 1 kG, measured at the poles on the surface of the star, was found insufficient for disk disruption.作者: Banister 時(shí)間: 2025-3-30 00:05 作者: 挑剔為人 時(shí)間: 2025-3-30 06:39
Hh 111 Stis Observations and Their Analysis Using Analytical and Numerical Modelsall bowshock within the jet beam. In this paper we present a long-slit spectrum of Herbig-Haro object HH 111 obtained with STIS and an interpretation of this observation in terms of an ejection velocity variability model.作者: 戲法 時(shí)間: 2025-3-30 10:22 作者: 認(rèn)為 時(shí)間: 2025-3-30 12:33 作者: flavonoids 時(shí)間: 2025-3-30 19:24 作者: BYRE 時(shí)間: 2025-3-30 22:59 作者: arterioles 時(shí)間: 2025-3-31 02:51
Ulcerative Colitis: An Autoimmune Disease? ulcerative colitis (8). Predominant IgG-containing immunocytes are observed in the lamina propria (9) and deposition of IgG and complement along the basement membrane of colonic epithelium in patients with ulcerative colitis (10) suggests formation of local immune complexes.
