PDF
PDF

Keywords

Black hole physics
stars: neutron
X-rays: binaries

How to Cite

Non-linear resonances in accretion disks and QPOs. (2004). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 20(1), 128-129. https://astronomia.unam.mx/journals/rmxac/article/view/2004rmxac..20..128k
hola

Abstract

Non-linear oscillations in the accretion disk are favored as an explanation of high-frequency QPOs observed in the light curves of low-mass X-ray binaries containing neutron stars, black holes, or white dwarfs.