1999A&A...343..197V


Query : 1999A&A...343..197V

1999A&A...343..197V - Astronomy and Astrophysics, volume 343, 197-201 (1999/3-1)

The phase-delay spectrum of GX5-1 on its normal branch.

VAUGHAN B.A., VAN DER KLIS M., LEWIN W.H.G., VAN PARADIJS J., MITSUDA K. and DOTANI T.

Abstract (from CDS):

We have measured the phase differences between X-ray intensity variations in different energy bands in data taken with Ginga of the Z source GX5-1 in its normal branch. We apply a χ2 optimal extraction technique to measure the phase-delay spectrum of the normal-branch quasi-periodic oscillations (QPO) and find a jump at 3.5keV. X-ray intensity variations at the QPO frequency in energy channels below 3.5keV are in phase with one another. The same is true of energy channels above 6keV. However, intensity variations in energy channels above 6keV lag those in channels below 3.5keV by ∼150°. We see no minimum in the fractional rms amplitude of the quasi-periodic oscillations at the jump energy, in contrast to what is seen in the Z source Cyg X-2, but because of limited statistics we cannot rule out such a minimum. We discuss our findings in the context of a radiation-hydrodynamics model for the normal-branch quasi-periodic oscillations.

Abstract Copyright:

Journal keyword(s): accretion, accretion disks - stars: individual: GX 5-1 - stars: neutron - X-rays: stars

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 V* V818 Sco LXB 16 19 55.0692669024 -15 38 25.017666540 11.60 12.40 11.1     Oev 1643 0
2 4U 1642-45 LXB 16 45 47.7 -45 36 40     14.30     ~ 417 1
3 4U 1758-25 LXB 18 01 09.7308060816 -25 04 44.120221284     11.08     ~ 655 1
4 V* V1341 Cyg LXB 21 44 41.1544345272 +38 19 17.066570988 15.00 15.13 14.68 15.00   A9III 1155 1

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