標(biāo)題: Titlebook: Accretion Disks — New Aspects; Proceedings of the E Emmi Meyer-Hofmeister,Henk Spruit Conference proceedings 1997 Springer-Verlag Berlin He [打印本頁] 作者: TUMOR 時(shí)間: 2025-3-21 19:16
書目名稱Accretion Disks — New Aspects影響因子(影響力)
書目名稱Accretion Disks — New Aspects影響因子(影響力)學(xué)科排名
書目名稱Accretion Disks — New Aspects網(wǎng)絡(luò)公開度
書目名稱Accretion Disks — New Aspects網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Accretion Disks — New Aspects被引頻次
書目名稱Accretion Disks — New Aspects被引頻次學(xué)科排名
書目名稱Accretion Disks — New Aspects年度引用
書目名稱Accretion Disks — New Aspects年度引用學(xué)科排名
書目名稱Accretion Disks — New Aspects讀者反饋
書目名稱Accretion Disks — New Aspects讀者反饋學(xué)科排名
作者: Interdict 時(shí)間: 2025-3-21 22:54
Super-eddington luminosity in the bursting pulsar GRO J1744-28. GRANAT/WATCH results,978-3-658-08930-6作者: interrogate 時(shí)間: 2025-3-22 03:52
Posterior Approach to Cervical Spineerved statistical properties. General relativistic calculations are also carried out. It appears that differences with the Newtonian case are weak, unless the hot source is very close to the black hole.作者: 易改變 時(shí)間: 2025-3-22 05:33
Jun Pan,Jun-xiang Peng,Song-tao Qicillation generated by viscous overstability could be seen at times near the outer boundary. Being confined there, the boundary layer remained almost stationary. However, for .=0.1 and large viscous speeds, short wavelength disturbances were seen throughout which could significantly affect the power作者: superfluous 時(shí)間: 2025-3-22 12:36
Morgan Schellenberg,Kenji Inabawo orders of magnitude. All of the bursts have similar profiles characterized by FWHM ～ 4 sec. The frequency of bursts also remained constant through the observations, 41±5 day. (after correction for the observations’ windowing). The WATCH flux measurements are completely unaffected by any dead-time作者: cringe 時(shí)間: 2025-3-22 14:49
Front Matterby a sum of poles and to determine their coupling constants and eventually also their masses. In nucleon-nucleon scattering this method has been applied for example by Bugg (l) and by Verwest et al. (2). With the advent of total cross-section data in pure spin states, however, it turned out by a det作者: spondylosis 時(shí)間: 2025-3-22 17:34
X-ray spectrum of low-mass X-ray binaries,bility of the labor markets, the link between marriage and childbearing, factors that help or hinder parents in balancing work and family obligations, gender equity, education systems, the housing markets, and governmental subsidies for the cost of childrearing.作者: mettlesome 時(shí)間: 2025-3-22 22:51
Black holes in X-ray binaries,ease of the thermal conductivity λ due to outward C0. diffusion followed by a fast increase of thermal conductivity in the first period (air in) and a slower but still important one in the latter stages (CFC-11 out). In the first period (1–10 weeks) a dissolution of the high molecular blowing agent 作者: 口音在加重 時(shí)間: 2025-3-23 01:26
GX 339-4: Hard X-ray observations; possible mechanism for transient outbursts, is the main user of high-potency sweeteners. After a fast growth between 1983 and 1990, the market for the low-calorie soft drinks has recently shown signs of slowing down. The increase in sales in the USA in the 1980s was in the two-digit region. However, recently diet sales showed a 9.2 and 2.6% 作者: 憤世嫉俗者 時(shí)間: 2025-3-23 06:30
X-ray spectrum of a disk illuminated by ions,ons that suit your business requirements...?..What You Will Learn..Understand low-code development and the factors driving its adoption.Solve your business‘s most pressing issues with Appsmith.Gain an understanding of the key concepts of app development, such as data management, APIs, troubleshootin作者: Outshine 時(shí)間: 2025-3-23 12:56
Anisotropic illumination of accretion disc in Seyfert I galaxies,n enhance traditional primary, secondary, and tertiary interventions in key behavioral and relational areas:.- Nutrition: weight/obesity control, diets, meal planning, vitamins and minerals, herbal supplements.- Exercise, expressive movement, relaxation, meditation, and mindfulness.- Writing for men作者: immunity 時(shí)間: 2025-3-23 16:17 作者: 極小量 時(shí)間: 2025-3-23 20:06 作者: 送秋波 時(shí)間: 2025-3-23 22:27
Modelling magnetised accretion discs,ntrator systems are discussed as well as a revolutionary idea of using mirrors in space in a sun-synchronous dawn–dusk polar orbit to provide sunbeams in the early morning and evening hours for large solar farms distributed around the world extending the available sunlight hours for these production作者: Hallmark 時(shí)間: 2025-3-24 02:24
Causal viscosity in accretion disc boundary layers,Kgauss. Superconducting magnets have been built using the alloys Nb.Sn and NbTi which produce fields of the order of 150 Kgauss and 80 Kgauss, respectively. These magnets offer something totally new to the area of electromotive machinery for the field energy and electromagnetic forces produced are o作者: Ptosis 時(shí)間: 2025-3-24 07:51
The nonlinear evolution of a single mode of the magnetic shearing instability,diation experiments and cases in surrounding forests after the CNPP accident for radiation effect studies of coniferous trees. By referring to them, the author explains the present situation and problems of the investigation on coniferous trees after the FNPP accident.作者: 可忽略 時(shí)間: 2025-3-24 14:12 作者: 不理會 時(shí)間: 2025-3-24 15:21 作者: 巨碩 時(shí)間: 2025-3-24 20:51 作者: NOCT 時(shí)間: 2025-3-25 01:31 作者: 結(jié)構(gòu) 時(shí)間: 2025-3-25 05:16
Radiation transfer in disks of CVs,ce1975. His research team at Boeing demonstrated the first GaAs/GaSb tandem concentrator solar cell in 1989 with a world record energy conversion efficiency of 35?, garnering awards from Boeing and NASA. He has978-3-031-30814-7978-3-031-30812-3作者: Substance 時(shí)間: 2025-3-25 10:10
Comparison of different models for the UV-X emission of AGN,r practical value explained..What You‘ll Learn.Low-Level Programming.?teaches programmers to:.Freely write in assembly language.Understand the programming model of Intel 64.Write maintainable and robust code in978-1-4842-2402-1978-1-4842-2403-8作者: Deject 時(shí)間: 2025-3-25 12:27 作者: octogenarian 時(shí)間: 2025-3-25 16:34
978-3-662-14142-7Springer-Verlag Berlin Heidelberg 1997作者: 健壯 時(shí)間: 2025-3-25 23:05
Accretion Disks — New Aspects978-3-540-68715-3Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: corpus-callosum 時(shí)間: 2025-3-26 00:54 作者: prostate-gland 時(shí)間: 2025-3-26 06:41
Morgan Schellenberg,Kenji Inabae involved and describe different models proposed to account for them. We schematize these models in a simple way, and compute the emitted spectra, insisting on their main characteristics and on their differences.作者: uncertain 時(shí)間: 2025-3-26 09:21 作者: Condyle 時(shí)間: 2025-3-26 12:59
Family Oziidae Dana, 1851 (Forceps Crabs) and those of X-ray binaries containing a black hole (black-hole XBs). The X-ray spectra of these systems change their characteristics with the mass accretion rate. At high X-ray luminosities, typically . .>10. erg sec., soft thermal emission from the accretion disk dominates. There is a distinct di作者: 懶鬼才會衰弱 時(shí)間: 2025-3-26 19:50
Anatomy of Craniocervical Junctionuring its four successive hard X-ray outbursts in 1990–1994 were studied in details. We suggest that the mechanism of GX 339-4 outbursts is triggering of the irradiation — driven instability in the low mass binary system.作者: Allodynia 時(shí)間: 2025-3-27 00:51 作者: Anhydrous 時(shí)間: 2025-3-27 04:56
Complications of Cervical Spine Surgery produces a comptonized spectrum with a shape that is only very weakly dependent on the incident energy flux and the distance from the accreting compact object, and is similar to observed spectra. Further evidence for ‘ion illuminated’ disks are the Li abundance in the secondaries of low mass X-ray 作者: 搏斗 時(shí)間: 2025-3-27 09:03 作者: Bricklayer 時(shí)間: 2025-3-27 13:15 作者: iodides 時(shí)間: 2025-3-27 17:12 作者: 確認(rèn) 時(shí)間: 2025-3-27 18:48 作者: Yourself 時(shí)間: 2025-3-28 00:37 作者: menopause 時(shí)間: 2025-3-28 04:22
Jun Pan,Jun-xiang Peng,Song-tao Qiity. The vertically integrated viscous stress relaxes towards its equilibrium value on a relaxation timescale ., which naturally yields a finite speed of propagation for viscous information. For a standard . prescription with . in the range 0.1 – 0.01, and ratio of viscous speed to sound speed in th作者: 搖曳 時(shí)間: 2025-3-28 06:24
Jun-xiang Peng,Yun Bao,Songtao Qibrium state is perturbed by adding a single eigenmode of the shearing instability and the subsequent evolution is followed into the nonlinear regime. Assuming that the perturbation is the most rapidly growing eigenmode, the linear theory remains applicable until the magnetic pressure perturbation is作者: Canopy 時(shí)間: 2025-3-28 11:13 作者: 廢墟 時(shí)間: 2025-3-28 18:18 作者: Evacuate 時(shí)間: 2025-3-28 20:42 作者: ETHER 時(shí)間: 2025-3-29 01:18
Gillian Morrison,Joshua M. Tobinnecessarily coplanar with the disc midplane..The calculations are relevant to a number of observed astrophysical phenomena, including the precession of jets associated with young stars, the high spectral index of some T Tauri stars, and the light curves of X-ray binaries such as Hercules X-1 which s作者: A保存的 時(shí)間: 2025-3-29 06:26 作者: 6Applepolish 時(shí)間: 2025-3-29 07:31 作者: 破裂 時(shí)間: 2025-3-29 14:27 作者: limber 時(shí)間: 2025-3-29 16:02 作者: 悅耳 時(shí)間: 2025-3-29 23:07
Jennifer Cone,Demetrios Demetriadesgenerally possess a sub-Keplerian angular momentum distribution and have maximum temperatures in the range 10. – 10. K. Accretion discs around rotating black holes are hotter and deposit less angular momentum on the central object than accretion discs around Schwarzschild black holes.作者: 討好女人 時(shí)間: 2025-3-30 03:28 作者: endocardium 時(shí)間: 2025-3-30 04:56
Anatomy of the Subaxial Cervical Spineal and short term variability characteristics of the hard X-ray emission were observed in the low spectral state of several black hole binaries. Possible relation of these variations with change of the mass accretion rate and low/high spectral state transitions is discussed.作者: 畏縮 時(shí)間: 2025-3-30 09:51
Complications of Cervical Spine Surgeryct object, and is similar to observed spectra. Further evidence for ‘ion illuminated’ disks are the Li abundance in the secondaries of low mass X-ray binaries and the 450 keV lines sometimes seen in black-hole transient spectra.作者: 陳舊 時(shí)間: 2025-3-30 16:11 作者: Agronomy 時(shí)間: 2025-3-30 19:15 作者: PATHY 時(shí)間: 2025-3-30 21:52
Basic Research in Craniopharyngiomanalysed quantitatively. Three-dimensional simulations are discussed, especially the resulting magnetic field structure. Possibilities of reproducing the field by an . dynamo are investigated, especially its symmetry with respect to the midplane.作者: amphibian 時(shí)間: 2025-3-31 00:55
Jun-xiang Peng,Yun Bao,Songtao QiAssuming that the perturbation is the most rapidly growing eigenmode, the linear theory remains applicable until the magnetic pressure perturbation is strong enough to induce significant deviations from the original density. If the initial perturbation is not the fastest growing mode, the faster growing modes will appear after some time.作者: 不吉祥的女人 時(shí)間: 2025-3-31 07:43
Apical 4 Chamber and Apical 5 Chamberand magnetic flux density distribution to be redistributed on the rather short orbital timescale, i.e. the dynamical timescale. As long as the instability works a significant fraction of the disk mass is accreted to the central object. After the instability the surface density decreases exponentially with disk radius.作者: 點(diǎn)燃 時(shí)間: 2025-3-31 12:20
Atlas of Critical Care Echocardiographyes control the radial advection of angular momentum. With buoyancy and turbulent diffusion, viscous and magnetic advection of angular momentum become comparable. All the magnetic disc solutions have eigenstate structures, corresponding to differing vertical variations of the field.作者: fibroblast 時(shí)間: 2025-3-31 14:02
Conference proceedings 1997ted by the X-UV spectra of AGN and their variability, the recent numerical simulations of magnetic fields in disks, the remarkable behavior of the superluminal source 1915+105 and the "bursting pulsar" 1744-28, to mention a few of the topics.作者: OMIT 時(shí)間: 2025-3-31 19:45
0075-8450 les presented by the X-UV spectra of AGN and their variability, the recent numerical simulations of magnetic fields in disks, the remarkable behavior of the superluminal source 1915+105 and the "bursting pulsar" 1744-28, to mention a few of the topics.978-3-662-14142-7978-3-540-68715-3Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: 帶來 時(shí)間: 2025-4-1 01:45
Family Oziidae Dana, 1851 (Forceps Crabs)the X-ray spectra of both systems undergo a transition to a hard power-law form. At further low luminosities (. .<10. erg sec.), the spectra become very soft. The characteristics of these X-ray spectra at different X-ray luminosities (different accretion rates) are described and the implications are discussed.作者: garrulous 時(shí)間: 2025-4-1 02:44 作者: 消滅 時(shí)間: 2025-4-1 09:10
Michelle F. Dawson,Alexis Salernotermined by obtaining a dispersion relation which is local in radius but is nevertheless capable of describing global normal modes. In particular, the stability boundary for the magnetorotational instability is obtained.作者: gangrene 時(shí)間: 2025-4-1 10:40 作者: FANG 時(shí)間: 2025-4-1 15:32 作者: 北極人 時(shí)間: 2025-4-1 21:46
