Titlebook: Oscillations of Disks; Shoji Kato Book 2016 Springer Japan 2016 Corotation Resonance.Discoseismology.Disk Oscillations.Epicyclic Frequenci

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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)絡公開度




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




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

Hyperopia

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.?.

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POINT

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.

清澈

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.

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evince

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.

Thyroiditis

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).

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