RXTE Studies of Long-Term X-ray Spectral Variations in 4U 1820-30
arXiv:astro-ph/0005496 · doi:10.1086/317019
Abstract
We present the results of detailed spectral studies of the ultra-compact low mass X-ray binary (LMXB) 4U 1820-30 carried out with the Rossi X-ray Timing Explorer (RXTE) during 1996-7. 4U 1820-30 is an ``atoll'' source X-ray burster (XRB) located in the globular cluster NGC 6624. It is known to have an 11 minute binary period and a ~176 day modulation in its 2--12 keV flux. Observations were made with the PCA and HEXTE instruments on RXTE at roughly one-month intervals to sample this long-term period and study flux-related spectral changes. There are clear correlations between our fitted spectral parameters and both the broad-band (2--50 keV) flux and the position in the color-color diagram, as described by the parameter S_a introduced by Mendez et al. (1999). In addition, we find a strong correlation between the position in the color-color diagram and the frequencies of the kilohertz quasi-periodic oscillations (kHz QPOs) reported by Zhang et al. (1998). This lends further support to the notion that evidence for the last stable orbit in the accretion disk of 4U 1820-30 has been observed. For a model consisting of Comptonization of cool photons by hot electrons plus an additional blackbody component, we report an abrupt change in the spectral parameters at the same accretion rate at which the kHz QPOs disappear. For a model consisting of a multicolor disk blackbody plus a cut-off power law, we find that the inner disk radius reaches a minimum at the same accretion rate at which the kHz QPO frequency saturates, as expected if the disk reaches the last stable orbit. Both models face theoretical and observational problems when interpreted physically for this system.
39 pages, 11 figures, accepted to the Astrophysical Journal
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Cited by in corpus (39)
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- Bright X-Ray Sources in M31 Globular Clusters
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- The Burst and Transient Source Experiment (BATSE) Earth Occultation Catalog of Low-Energy Gamma-Ray Sources
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- The nature of the Island and Banana States in Atoll sources and a Unified Model for Low Mass X-ray Binaries
- On the multi-periodicities in the X-ray dipper XB 1916-053
- The Island state of the Atoll Source 4U 1820--30
- Dependence of the orbital modulation of X-rays from 4U 1820-303 on the accretion rate
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- ALMA observations of 4U 1728-34 and 4U 1820-30: first detection of neutron star X-ray binaries at 300 GHz
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- ASCA Observations of GX 354-0 and KS 1731-260
- Spectral state evolution of 4U~1820-30: the stability of the spectral index of Comptonization tail
- Simultaneous X-ray/optical observations of GX 9+9 (4U 1728-16)
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- The MAVERIC Survey: Variable Jet-Accretion Coupling in Luminous Accreting Neutron Stars in Galactic Globular Clusters
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- BeppoSAX observations of two unclassified LMXBs: X1543-624 and X1556-605
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- The INTEGRAL long monitoring of persistent Ultra Compact X-ray Bursters
- An XTE Archival Search for Coherent X-ray Pulsations in LMXB 4U 1820-30
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- ROSAT/Chandra Observations of a Bright Transient in M81
- X-ray Timing beyond the Rossi X-ray Timing Explorer