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24 April 2024
 
  » arxiv » astro-ph/9806052

 Article overview


Evolution of AQL X-1 During the Rising Phase of its 1998 Outburst
Wei Cui ; Didier Barret ; S. N. Zhang ; Wan Chen ; Laurence Boirin ; Jean Swank ;
Date 3 Jun 1998
Subject astro-ph
Affiliation MIT, CESR, MSFC, GSFC
AbstractWe present results from 16 snapshots of Aql X-1 with RXTE during the rising phase of its recent outburst. The observations were carried out at a typical rate of once or twice per day. The source shows interesting spectral evolution during this period. Phenomenologically, it bears remarkable similarities to ``atoll’’ sources. Shortly after the onset of the outburst, the source is seen to be in an ``island’’ state, but with little X-ray variability. It then appears to have made a rapid spectral transition (on a time scale less than half a day) to another ``island’’ state, where it evolves slightly and stays for 4 days. In this state, the observed X-ray flux becomes increasingly variable as the source brightens. Quasi-period oscillation (QPO) in the X-ray intensity is detected in the frequency range 670--870 Hz. The QPO frequency increases with the X-ray flux while its fractional rms decreases. The QPO becomes undetectable following a transition to a ``banana’’ state, where the source continues its evolution by moving up and down the ``banana’’ branch in the color-color diagram as the flux (presumably, the mass accretion rate) fluctuates around the peak of the outburst. Throughout the entire period, the power density spectrum is dominated by very-low frequency noises. Little power can be seen above ~1 Hz, which is different from typical ``atoll’’ sources. In the ``banana’’ state, the overall X-ray variability remains low (with fractional rms ~3--4%) but roughly constant. The observed X-ray spectrum is soft with few photons from above $sim$25 keV, implying the thermal origin of the emission. The evolution of both spectral and temporal X-ray properties is discussed in the context of disk-instability models.
Source arXiv, astro-ph/9806052
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