標(biāo)題: Titlebook: Exploring the Universe: From Near Space to Extra-Galactic; A Collection of Rese Banibrata Mukhopadhyay,Sudipta Sasmal Conference proceeding [打印本頁(yè)] 作者: mobility 時(shí)間: 2025-3-21 18:33
書目名稱Exploring the Universe: From Near Space to Extra-Galactic影響因子(影響力)
書目名稱Exploring the Universe: From Near Space to Extra-Galactic影響因子(影響力)學(xué)科排名
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書目名稱Exploring the Universe: From Near Space to Extra-Galactic網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Exploring the Universe: From Near Space to Extra-Galactic被引頻次
書目名稱Exploring the Universe: From Near Space to Extra-Galactic被引頻次學(xué)科排名
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書目名稱Exploring the Universe: From Near Space to Extra-Galactic年度引用學(xué)科排名
書目名稱Exploring the Universe: From Near Space to Extra-Galactic讀者反饋
書目名稱Exploring the Universe: From Near Space to Extra-Galactic讀者反饋學(xué)科排名
作者: 外面 時(shí)間: 2025-3-21 23:32 作者: DIS 時(shí)間: 2025-3-22 01:44 作者: Cognizance 時(shí)間: 2025-3-22 07:18
Exploring the Universe: From Near Space to Extra-Galactic978-3-319-94607-8Series ISSN 1570-6591 Series E-ISSN 1570-6605 作者: Lethargic 時(shí)間: 2025-3-22 09:03
Dai Phu Huynh,Chaoliang He,Doo Sung Leeed to be rotating, however be the magnitude of angular speed. The generalized astrophysical black hole is the rotating one (the Kerr black hole) which often accretes matter from its surrounding (e.g. from its binary companion) forming an accretion disk (namely X-ray binary). This accretion disk is t作者: 離開可分裂 時(shí)間: 2025-3-22 15:35
Aristeidis Papagiannopoulos,Stergios Pispasnt from terrestrial versions. The temperature can range from relativistic values to non-relativistic ones and at high temperature, the fluid is composed of charges and not neutral particles as is the case in the terrestrial version..We use relativistic equation of state to describe trans-relativisti作者: 離開可分裂 時(shí)間: 2025-3-22 18:46
Yoshihito Osada,Ryuzo Kawamura,Ken-Ichi Sanos has evolved from a static Keplerian disk to modern days dynamic advective flow models. As a result, the images of black holes have changed. Major efforts of producing simulated black hole images are briefly presented. Distinguishing event horizon from the disk will be one of the major discoveries 作者: LAVA 時(shí)間: 2025-3-23 00:34
Hydrogen Production from Recycled Gases,binary systems of compact objects. An example of such a system is a stellar mass compact star (typically a neutron star or a black hole) orbiting a central super-massive black hole embedded in a massive accretion disk. We particularly focus on the effects produced by hydrodynamic drag of the disk on作者: maverick 時(shí)間: 2025-3-23 02:56 作者: 常到 時(shí)間: 2025-3-23 05:31 作者: barium-study 時(shí)間: 2025-3-23 10:18
Hui Wang,Dan-Wei Zhang,Zhan-Ting Li jets and outflows which are also important components of black hole system. In recent times it has been reported that beside spin of the black hole, another parameter may be playing crucial role in determining the origin and acceleration of outflows and jets. The strength of centrifugal pressure su作者: modifier 時(shí)間: 2025-3-23 16:48 作者: 眼界 時(shí)間: 2025-3-23 19:30 作者: cancer 時(shí)間: 2025-3-24 00:53 作者: 懦夫 時(shí)間: 2025-3-24 05:12 作者: 合適 時(shí)間: 2025-3-24 10:24
Hydrogen: The Ultimate Energy Sourceow towards the compact object. There are two components that dominate the accretion flow onto black holes, one having Keplerian angular momentum distribution near equatorial plane, another low angular momentum sub-Keplerian flow surrounding the Keplerian flow. A sudden rise in viscosity in the accre作者: 高度表 時(shí)間: 2025-3-24 13:37 作者: ADOPT 時(shí)間: 2025-3-24 18:21 作者: IVORY 時(shí)間: 2025-3-24 21:44 作者: 鴿子 時(shí)間: 2025-3-25 01:38 作者: 手段 時(shí)間: 2025-3-25 05:05 作者: 偽造 時(shí)間: 2025-3-25 09:57 作者: ABASH 時(shí)間: 2025-3-25 13:30 作者: 影響深遠(yuǎn) 時(shí)間: 2025-3-25 16:43
Hydrogen Production from Recycled Gases,tional wave signal emitted from such systems. On the other hand, by studying the emitted gravitational wave signals profile, one could infer about the nature of the accretion disk, which has been, till date, done only by observing the electro-magnetic signals coming from it. This multi-messenger ast作者: precede 時(shí)間: 2025-3-25 23:33
Aleksander Koll,Peter Wolschannly, we calculate the critical values of both viscosity and accretion rate that cater shocks. We continue the search of shocked accretion solutions for two-temperature flow and obtain such solutions for the first time in the literature. Finally, we discuss the possible origin of mass loss from the ac作者: Aerate 時(shí)間: 2025-3-26 00:11 作者: 不來(lái) 時(shí)間: 2025-3-26 04:31
Han Myoung Lee,N. Jiten Singh,Kwang S. Kiman 0.008, all sources were categorized in hard spectral state. When it was in the ranges 0.008–0.035 and 0.035–0.01, hard and soft intermediate states were observed respectively. Soft spectral state would be expected for any larger values of . in the sub-Keplerian component. Thus the concept of visc作者: 艦旗 時(shí)間: 2025-3-26 09:16
Hydrogen: The Ultimate Energy Sourcee an advective halo. We believe that, for the first time, our results are able to simulate the two-component advective flow dynamics during an entire X-ray outburst of a black hole candidate. Also, we see, the hysteresis effect of an outburst is caused mainly for the difference in the time duration 作者: Dislocation 時(shí)間: 2025-3-26 14:57
https://doi.org/10.1007/978-0-85729-136-3cularly true for weakly viscous, low angular momentum transonic or advective discs. We focus our study to the trajectories of toroidal flux tubes inside a geometrically thick flow which undergoes a centrifugal force supported shock and also the effects of these flux tubes on the dynamics of the infl作者: 共同時(shí)代 時(shí)間: 2025-3-26 17:07 作者: 衣服 時(shí)間: 2025-3-26 22:02
Relativistic Flows in Astrophysics for magnetically driven outflows. We show that the flow geometry close to a black hole is quite different from a neutron star because of the strong magnetic field around the latter, which has implication on the radiative processes dominant nearby. We also obtained shock solutions for lepton dominat作者: Enliven 時(shí)間: 2025-3-27 02:03
Gravitational Wave Emission from Binary Mergers: Ideal Versus Real Picturetional wave signal emitted from such systems. On the other hand, by studying the emitted gravitational wave signals profile, one could infer about the nature of the accretion disk, which has been, till date, done only by observing the electro-magnetic signals coming from it. This multi-messenger ast作者: POINT 時(shí)間: 2025-3-27 05:35 作者: 修飾語(yǔ) 時(shí)間: 2025-3-27 12:01 作者: 嫻熟 時(shí)間: 2025-3-27 16:35 作者: Demonstrate 時(shí)間: 2025-3-27 19:57 作者: Confidential 時(shí)間: 2025-3-27 22:44 作者: 怪物 時(shí)間: 2025-3-28 03:58
1570-6591 fthe research topics pursued by Chakrabarti’s fifty odd doctoral students, many of whom have become renowned scientists in their own right, after starting with a certain subject under Chakrabarti and then migra978-3-030-06883-7978-3-319-94607-8Series ISSN 1570-6591 Series E-ISSN 1570-6605 作者: 陳腐思想 時(shí)間: 2025-3-28 08:00 作者: Acetaldehyde 時(shí)間: 2025-3-28 11:37 作者: Fluctuate 時(shí)間: 2025-3-28 17:53
Monte-Carlo Simulation as a Defining Tool to Diagnose Timing and Spectral Properties of Flows Aroundm is a classic example where Monte-Carlo simulation has been found to be very useful. This Chapter deals with the schematics that have been utilized. Spectral variations with various parameters are shown.作者: 巨大沒有 時(shí)間: 2025-3-28 19:12
Conference proceedings 2018 contributions by about fifty scientists who work on diverse topics in contemporary astrophysics and space science including new and low-cost balloon borne experiments, planetary science, astrochemistry and the origin of life, ionospheric research and earthquake predictions, relativistic astrophysic作者: 易碎 時(shí)間: 2025-3-29 00:31 作者: 粘連 時(shí)間: 2025-3-29 05:15 作者: 打谷工具 時(shí)間: 2025-3-29 11:14 作者: Commemorate 時(shí)間: 2025-3-29 11:24 作者: Femish 時(shí)間: 2025-3-29 17:17
https://doi.org/10.1007/978-94-011-0111-0y to study simultaneously the time dependence of the disk structure and its spectral as well as temporal properties. We prove several of the conjectures that were made earlier based on theoretical studies and other simulations. We also discuss the current developments in this simulation code and the future scopes.作者: 宴會(huì) 時(shí)間: 2025-3-29 23:36 作者: OUTRE 時(shí)間: 2025-3-30 03:19
Evolution of Imaging of Black Hole Accretion-Outflow System over Half a Centuryof this century. Event Horizon Telescope (EHT) is getting prepared to discern the horizon of Sgr A* where radio interferometry technique has been deployed. For Galactic black holes, the required resolution is much higher and X-ray interferometry is essential.作者: 身心疲憊 時(shí)間: 2025-3-30 06:15
On the Nature of Outflows from Low Angular Momentum Inflows Around Black Holespported shock wave in case of low angular momentum flow around black holes may be responsible for jets and outflows. The energy dissipation as well as mass loss rate across the shock may happen at the base of the jets and outflows. The outflow properties are determined by these parameters close to the black hole.作者: 輕彈 時(shí)間: 2025-3-30 09:13
Generalized Flows Around Neutron Starse NSs. We showcase some of our findings from Monte Carlo and Smoothed Particle Hydrodynamic simulations which further strengthens the points raised in Sect. 4. In summary, we remark on the possibility of future works using TCAF for both weakly magnetic and magnetic Neutron Stars.作者: 類人猿 時(shí)間: 2025-3-30 15:45
Formation of Two Component Flows by Numerical Simulations Around Black Holesway from the equatorial plane behaves like a transonic flow with standing and oscillating shocks. Finally, we observed that, our solution is consistent with the Chakrabarti-Titarchuk two-component advective flow configuration as the flow approaches to a black hole.作者: CHASE 時(shí)間: 2025-3-30 19:04 作者: 參考書目 時(shí)間: 2025-3-31 00:37 作者: 法律的瑕疵 時(shí)間: 2025-3-31 02:16 作者: Pillory 時(shí)間: 2025-3-31 05:39
Radiation Characteristics of Two-Component Accretion Flow Paradigm Around Black Holesermassive black holes. Also, two-component advective solutions can be used to understand the triggering of outburst events in compact X-ray sources due to sudden surge of viscosity or mass accretion at the outer boundary.作者: nuclear-tests 時(shí)間: 2025-3-31 13:13 作者: 可卡 時(shí)間: 2025-3-31 14:44 作者: arthrodesis 時(shí)間: 2025-3-31 20:05
Spinning Black Holes, Spinning Flows and Spinorsed to be rotating, however be the magnitude of angular speed. The generalized astrophysical black hole is the rotating one (the Kerr black hole) which often accretes matter from its surrounding (e.g. from its binary companion) forming an accretion disk (namely X-ray binary). This accretion disk is t作者: chisel 時(shí)間: 2025-3-31 23:06 作者: GRIN 時(shí)間: 2025-4-1 04:10
Evolution of Imaging of Black Hole Accretion-Outflow System over Half a Centurys has evolved from a static Keplerian disk to modern days dynamic advective flow models. As a result, the images of black holes have changed. Major efforts of producing simulated black hole images are briefly presented. Distinguishing event horizon from the disk will be one of the major discoveries 作者: Aesthete 時(shí)間: 2025-4-1 06:02
Gravitational Wave Emission from Binary Mergers: Ideal Versus Real Picturebinary systems of compact objects. An example of such a system is a stellar mass compact star (typically a neutron star or a black hole) orbiting a central super-massive black hole embedded in a massive accretion disk. We particularly focus on the effects produced by hydrodynamic drag of the disk on
