A Resonance Model of Quasi-Periodic Oscillations of Low-Mass X-Ray Binaries

Publications of the Astronomical Society of Japan

Kato, Shoji¹ 

[1] Department of Informatics, Nara Sangyo University, Ikoma-gun, Nara 636-8503 ,

关键词: "accretion;    accrection disks";    "hectohertz QPOs";    "horizontal branch QPOs";    "kHz QPOs";    "relativistic processes";    resonance;    warp;    "X-rays: stars";   

DOI  :  10.1093/pasj/57.3.L17

学科分类：天文学(综合)

来源: Oxford University Press

【 摘 要 】

Wetrytounderstandthequasi-periodicoscillations(QPOs)inlow-massneutron-starandblack-holeX-raybinariesbyaresonancemodelinwarpeddiskswithprecession.Ourmainconcernishigh-frequencyQPOs,hectohertzQPOs,andhorizontal-branchQPOsinthezsourcesandtheatollsources,andthecorrespondingQPOsinblack-holeX-raybinaries.Ourresonancemodelcanqualitatively,butsystematically,explaintheseQPOsbyregardinghectohertzQPOsasaprecessionofwarp.

【 授权许可】

Unknown