Discovery of a new, third kilohertz quasi-periodic oscillation in 4U 1608-52, 4U 1728-34, and 4U 1636-53.: Sidebands to the lower kilohertz quasi-periodic oscillation?

被引:49
作者
Jonker, PG
Méndez, M
Van der Klis, M
机构
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
[2] Ctr High Energy Astrophys, NL-1098 SJ Amsterdam, Netherlands
[3] Natl Univ La Plata, Fac Ciencias Astron & Geofis, RA-1900 La Plata, Argentina
关键词
accretion; accretion disks; stars : individual (4U 1608-52; 4U; 1636-53; 1728-34); stars : neutron; X-rays : stars;
D O I
10.1086/312871
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a third kilohertz quasi-periodic oscillation (kHz QPO) in the power spectra of the low-mass X-ray binaries 4U 1608-52 (6.3 sigma), 4U 1728-34 (6.0 sigma), and 4U 1636-53 (3.7 sigma) which is present simultaneously with the previously known kHz QPO pair. The new kHz QPO is found at a frequency that is 52.8 +/- 0.9, 64 +/- 2, and 58.4 +/- 1.9 Hz higher than the frequency of the lower kHz QPO in 4U 1608-52, 4U 1728-34, and 4U 1636-53, respectively. The difference between the frequency of the new kHz QPO and the lower kHz QPO increased in 4U 1608-52 from 49.6 +/- 1.4 to 53.9 +/- 0.5 Hz when the frequency of the lower kHz QPO increased from 672 to 806 Hz. Simultaneously the difference between the frequency of the new kHz QPO and the upper kHz QPO increased by similar to 60 Hz, suggesting that the new Wt QPO is unrelated to the upper kHz QPO. In 4U 1636-53 a fourth, weaker, kHz QPO is simultaneously detected (3 sigma) at the same frequency separation below the lower Wt QPO, suggesting that the new kHz QPOs are sidebands to the lower kHz QPO. We discuss the nature of this new kHz QPO and its implications on the models for the kHz QPOs.
引用
收藏
页码:L29 / L32
页数:4
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