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標題: Titlebook: Oscillations of Disks; Shoji Kato Book 2016 Springer Japan 2016 Corotation Resonance.Discoseismology.Disk Oscillations.Epicyclic Frequenci [打印本頁]

作者: Sparkle 時間: 2025-3-21 16:18
書目名稱Oscillations of Disks影響因子(影響力)

書目名稱Oscillations of Disks影響因子(影響力)學科排名

書目名稱Oscillations of Disks網(wǎng)絡(luò)公開度

書目名稱Oscillations of Disks網(wǎng)絡(luò)公開度學科排名

書目名稱Oscillations of Disks被引頻次

書目名稱Oscillations of Disks被引頻次學科排名

書目名稱Oscillations of Disks年度引用

書目名稱Oscillations of Disks年度引用學科排名

書目名稱Oscillations of Disks讀者反饋

書目名稱Oscillations of Disks讀者反饋學科排名

作者: Hyperopia 時間: 2025-3-21 23:13
Wave-Wave Resonant Instability in Deformed Diskso et?al. (Publ Astron Soc Jpn 63:363, 2011)) formulated the instability in a perspective way. In this chapter, we outline the formulation by Kato (Publ Astron Soc Jpn 65:75, 2013). Applications to time variations in dwarf novae and X-ray binaries are presented in Chap.?.

作者: llibretto 時間: 2025-3-22 01:53

作者: ingenue 時間: 2025-3-22 08:20

作者: POINT 時間: 2025-3-22 11:08
Frequencies of Trapped Oscillations and Applicationwtonian disks are examined. The oscillation modes examined are one-armed p-mode (one-armed precession mode) and one-armed vertical p-mode (tilt mode). The results are examined whether they can describe positive and negative superhumps in dwarf novae.

作者: 清澈 時間: 2025-3-22 16:07
Introductionions in accretion disks, focusing on those which will be related to disk oscillations. The main oscillatory phenomena which we focus our attention are V/R variations in Be stars, positive and negative superhumps in dwarf novae, high-frequency quasi-periodic oscillations in neutron-star and black-hole X-ray binaries.

作者: concentrate 時間: 2025-3-22 20:08

作者: evince 時間: 2025-3-23 00:03
Wave-Wave Resonant Instability in Deformed Disks: Applicationserhumps. Furthermore, some oscillatory phenomena in X-ray sources might be attributed to this process. In this context we present here attempts to apply the process to describing high-frequency QPOs in X-ray sources, in addition to superhumps.

作者: Thyroiditis 時間: 2025-3-23 01:34
Corotation Instabilitystron Soc 208:721, 1984) (see Chap.?.). This work by Paparoizou and Pringle stimulated many subsequent studies on corotation instability in tori and disks. In this chapter, we will describe the essence of corotation instability in geometrically thin disks by presenting Drury’s work (Mon Not R Astron Soc 217:821, 1985).

作者: 嘴唇可修剪 時間: 2025-3-23 06:14

作者: FRET 時間: 2025-3-23 11:47

作者: ANA 時間: 2025-3-23 16:51
Derivation of Linear Wave Equations and Wave Energylerian descriptions. The former is better to examine some basic properties of oscillations, but the latter is convenient to study practical problems. In addition to wave equation, in this chapter, we derive expressions for wave energy, since the wave energy is one of important quantities which are c

作者: Occipital-Lobe 時間: 2025-3-23 18:09
Vertical Oscillations. We shall study the characteristics of equation?(.) step by step by considering some idealized cases. First, in this chapter, we consider purely vertical oscillations, although such oscillations are not realized in actual disk systems, since the pressure variation associated with these oscillations

作者: prediabetes 時間: 2025-3-24 00:42

作者: 氣候 時間: 2025-3-24 05:27

作者: GUEER 時間: 2025-3-24 08:37
Frequencies of Trapped Oscillations and Applicationxamine whether they can describe periodic or quasi-periodic oscillations observed in X-ray binaries and dwarf novae. First, we examine frequencies of p-mode, c-mode, and vertical p-mode oscillations trapped in the innermost regions of relativistic disks. The results are compared with the high-freque

作者: medium 時間: 2025-3-24 14:39

作者: amnesia 時間: 2025-3-24 17:24

作者: Tincture 時間: 2025-3-24 19:55

作者: Enrage 時間: 2025-3-25 00:45
Wave-Wave Resonant Instability in Deformed Disksave resonant excitation in deformed disks. Disk deformation from axisymmetric state is widely expected in tidally deformed disks. Even in a single star, long-living (time-periodic) deformations may be present on disks (e.g., warps). Basics on a wave-wave resonant instability in deformed disks was st

作者: 可觸知 時間: 2025-3-25 07:12

作者: 有權(quán)威 時間: 2025-3-25 10:29
Sonic Point Instability and Stochastic Excitation of Oscillations by Turbulencease of relativistic disks, the accretion flows fall to central objects by passing a sonic point. In the case where the sonic point is a nodal-type critical point, accretion flows are locally unstable at the sonic point and waves propagating both inward and outward are generated there. This is an int

作者: foliage 時間: 2025-3-25 11:41

作者: 善辯 時間: 2025-3-25 16:57
range of effective temperatures from 14 200 K down to 11400 K. Comparison with mixing length theory (MLT) yields a conflicting picture: The dynamics of convection is not governed by up- and downflowing bubbles which dissolve after travelling some characteristic distance - but by the formation, advec

作者: 無能的人 時間: 2025-3-25 23:35

作者: 概觀 時間: 2025-3-26 02:01
Shoji Katorange of effective temperatures from 14 200 K down to 11400 K. Comparison with mixing length theory (MLT) yields a conflicting picture: The dynamics of convection is not governed by up- and downflowing bubbles which dissolve after travelling some characteristic distance - but by the formation, advec

作者: 射手座 時間: 2025-3-26 05:05
Shoji Katorange of effective temperatures from 14 200 K down to 11400 K. Comparison with mixing length theory (MLT) yields a conflicting picture: The dynamics of convection is not governed by up- and downflowing bubbles which dissolve after travelling some characteristic distance - but by the formation, advec

作者: Amylase 時間: 2025-3-26 10:13
Shoji Katorange of effective temperatures from 14 200 K down to 11400 K. Comparison with mixing length theory (MLT) yields a conflicting picture: The dynamics of convection is not governed by up- and downflowing bubbles which dissolve after travelling some characteristic distance - but by the formation, advec

作者: 伴隨而來 時間: 2025-3-26 13:40

作者: Polydipsia 時間: 2025-3-26 19:13
Shoji Katorange of effective temperatures from 14 200 K down to 11400 K. Comparison with mixing length theory (MLT) yields a conflicting picture: The dynamics of convection is not governed by up- and downflowing bubbles which dissolve after travelling some characteristic distance - but by the formation, advec

作者: Fibrin 時間: 2025-3-26 22:54

作者: palette 時間: 2025-3-27 04:49
Shoji Katorange of effective temperatures from 14 200 K down to 11400 K. Comparison with mixing length theory (MLT) yields a conflicting picture: The dynamics of convection is not governed by up- and downflowing bubbles which dissolve after travelling some characteristic distance - but by the formation, advec

作者: 流浪者 時間: 2025-3-27 08:00

作者: 滴注 時間: 2025-3-27 10:34

作者: Vasoconstrictor 時間: 2025-3-27 16:12
Shoji Katorange of effective temperatures from 14 200 K down to 11400 K. Comparison with mixing length theory (MLT) yields a conflicting picture: The dynamics of convection is not governed by up- and downflowing bubbles which dissolve after travelling some characteristic distance - but by the formation, advec

作者: anchor 時間: 2025-3-27 20:33
Shoji Katorange of effective temperatures from 14 200 K down to 11400 K. Comparison with mixing length theory (MLT) yields a conflicting picture: The dynamics of convection is not governed by up- and downflowing bubbles which dissolve after travelling some characteristic distance - but by the formation, advec

作者: 解凍 時間: 2025-3-28 01:35

作者: inquisitive 時間: 2025-3-28 04:20

作者: 閑蕩 時間: 2025-3-28 10:13
range of effective temperatures from 14 200 K down to 11400 K. Comparison with mixing length theory (MLT) yields a conflicting picture: The dynamics of convection is not governed by up- and downflowing bubbles which dissolve after travelling some characteristic distance - but by the formation, advec

作者: insolence 時間: 2025-3-28 11:28
Oscillations of Disks978-4-431-56208-5Series ISSN 0067-0057 Series E-ISSN 2214-7985

作者: RAG 時間: 2025-3-28 17:58

作者: 格言 時間: 2025-3-28 19:06
Shoji KatoExplains the current state of disk-oscillation theory, providing a potentially important tool to accurately determine spins of black hole sources in the universe.Clarifies our current understanding of

作者: 構(gòu)想 時間: 2025-3-29 00:07