2010ApJ...710..836Q


Query : 2010ApJ...710..836Q

2010ApJ...710..836Q - Astrophys. J., 710, 836-842 (2010/February-2)

The energy dependence of the centroid frequency and phase lag of the quasi-periodic oscillations in GRS 1915+105.

QU J.L., LU F.J., LU Y., SONG L.M., ZHANG S., DING G.Q. and WANG J.M.

Abstract (from CDS):

We present a study of the centroid frequencies and phase lags of quasi-periodic oscillations (QPOs) as functions of photon energy for GRS 1915+105. It is found that the centroid frequencies of the 0.5-10 Hz QPOs and their phase lags are both energy dependent, and there exists an anticorrelation between the QPO frequency and phase lag. These new results challenge the popular QPO models, because none of them can fully explain the observed properties. We suggest that the observed QPO phase lags are partially due to the variation of the QPO frequency with energy, especially for those with frequency higher than 3.5 Hz.

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Journal keyword(s): accretion, accretion disks - black hole physics - stars: individual: GRS 1915+105 - stars: oscillations

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* V381 Nor HXB 15 50 58.6637920704 -56 28 35.258385000           K3III 1254 0
2 V* V1033 Sco HXB 16 54 00.1423963019 -39 50 44.761701340       16.14   F3-6IV 1980 0
3 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2810 0

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