Discovery of microsecond time lags in kilohertz QPOs

被引:35
作者
Vaughan, BA
VanderKlis, M
Mendez, M
VanParadijs, J
Wijnands, RAD
Lewin, WHG
Lamb, FK
Psaltis, D
Kuulkers, E
Oosterbroek, T
机构
[1] UNIV AMSTERDAM,ASTRON INST ANTON PANNEKOEK,NL-1098 SJ AMSTERDAM,NETHERLANDS
[2] NATL INST NUCL & HIGH ENERGY PHYS,CTR HIGH ENERGY ASTROPHYS,NL-1098 SJ AMSTERDAM,NETHERLANDS
[3] MIT,CAMBRIDGE,MA 02139
[4] UNIV ILLINOIS,DEPT PHYS & ASTRON,URBANA,IL 61801
[5] UNIV OXFORD,NUCL & ASTROPHYS LAB,OXFORD OX1 3RH,ENGLAND
[6] EUROPEAN SPACE AGCY,ESTEC,DEPT SPACE SCI,DIV ASTROPHYS,NL-2200 AG NOORDWIJK,NETHERLANDS
[7] NATL UNIV LA PLATA,FAC CIENCIAS ASTRON & GEOFIS,RA-1900 LA PLATA,ARGENTINA
[8] UNIV ALABAMA,DEPT PHYS,HUNTSVILLE,AL 35899
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
accretion; accretion disks; stars; individual; (4U; 1608-52; 4U; 0614+614; 1636-53); neutron; X-rays;
D O I
10.1086/310740
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using the Rossi X-Ray Timing Explorer, we have measured similar to 27 mu s time delays in 830 Hz quasi-periodic oscillations (QPOs) between 4-6 and 11-17 keV in 4U 1608-52, with high-energy photons lagging low-energy photons, and found upper limits to the time delays of 45 mu s between 2-6.5 and 6.5-67 keV in similar to 730 Hz QPOs in 4U 0614+091 and 30 mu s between 8.7-12.4 and 12.4-67 keV in similar to 870 Hz QPOs in 4U 1636-53. We also find that the cross-coherence function between QPOs at different energies is greater than 0.85 with 95% confidence in 4U 1608-52 and 4U 1636-53. If Compton upscattering of low-energy X-rays in a region with an optical depth of a few is responsible for the delays, then the Compton upscattering region is between a few kilometers and a few tens of kilometers in size.
引用
收藏
页码:L115 / L118
页数:4
相关论文
共 29 条
[1]   IS GX5-1 A MILLISECOND PULSAR [J].
ALPAR, MA ;
SHAHAM, J .
NATURE, 1985, 316 (6025) :239-241
[2]   Discovery of 800 Hz quasi-periodic oscillations in 4U 1608-52 [J].
Berger, M ;
vanderKlis, M ;
vanParadijs, J ;
Lewin, WHG ;
Lamb, F ;
Vaughan, B ;
Kuulkers, E ;
Augusteijn, T ;
Zhang, W ;
Marshall, FE ;
Swank, JH ;
Lapidus, I ;
Lochner, JC ;
Strohmayer, TE .
ASTROPHYSICAL JOURNAL, 1996, 469 (01) :L13-&
[3]  
BRADT HV, 1993, ASTRON ASTROPHYS SUP, V97, P355
[4]  
BRANDT S, 1992, ASTRON ASTROPHYS, V262, pL15
[5]   THE EFFECT OF A HOT, SPHERICAL SCATTERING CLOUD ON QUASI-PERIODIC OSCILLATION BEHAVIOR [J].
BUSSARD, RW ;
WEISSKOPF, MC ;
ELSNER, RF ;
SHIBAZAKI, N .
ASTROPHYSICAL JOURNAL, 1988, 327 (01) :284-293
[6]  
DIETERS S, 1997, UNPUB
[7]  
KYLAFIS ND, 1989, NATO ADV SCI I C-MAT, V262, P731
[8]  
Lamb F. K., 1988, Advances in Space Research, V8, P421, DOI 10.1016/0273-1177(88)90440-1
[9]   QUASI-PERIODIC OSCILLATIONS IN BRIGHT GALACTIC-BULGE X-RAY SOURCES [J].
LAMB, FK ;
SHIBAZAKI, N ;
ALPAR, MA ;
SHAHAM, J .
NATURE, 1985, 317 (6039) :681-687
[10]  
LAMB FK, 1989, ESA, P215