Abstract
We have studied the 1999 soft X-ray transient outburst of XTE J1859+226 at radio and X-ray wavelengths. The event was characterized by strong variability in the disc, corona and jet - in particular, a number of radio flares (ejections) took place and seemed well-correlated with hard X-ray events. Apparently unusual for the canonical `soft' X-ray transient, there was an initial period of low/hard state behaviour during the rise from quiescence but prior to the peak of the main outburst - we show that not only could this initial low/hard state be a ubiquitous feature of soft X-ray transient outbursts, but also it could be extremely important in our study of outburst mechanisms.
Original language | English |
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Pages (from-to) | 765-775 |
Number of pages | 11 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 331 |
Publication status | Published - 2002 |
Keywords
- accretion
- accretion discs
- stars: individual: XTE J1859+226
- X-rays: stars