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Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/1534
- Title
- The 2003 radio outburst of a new X-ray transient: XTE J1720-318
- Author(s)
- Brocksopp, Catherine; Corbel, Stephane; Fender, Robert P.; Rupen, M.; Sault, R.; Tingay, Steven J.; Hannikainen, D.; O'Brien, K.
- Abstract
- We present radio observations of the black hole X-ray transient XTE J1720−318, which was discovered in 2003 January as it entered an outburst. We analyse the radio data in the context of the X-ray outburst and the broad-band spectrum. An unresolved radio source was detected during the rising phase, reaching a peak of nearly 5 mJy approximately coincident with the peak of the X-ray light curve. A study of the spectral indices suggests that at least two ejection events took place, with the radio-emitting material expanding and becoming optically thin as it faded. The broad-band spectra suggested that the accretion disc dominated the emission, as expected for a source in a soft state. The radio emission decayed to below the sensitivity of the telescopes for 6 weeks but switched on again during the transition of the X-ray source to the low/hard state. At least one 'glitch' was superimposed on the otherwise exponential decay of the X-ray light curve, which was reminiscent of the multiple jet ejections of XTE J1859+226. We also present a Ks-band image of XTE J1720−318 and its surrounding field taken with the Very Large Telescope.
- Publication type
- Journal article
- Research centre
- Swinburne University of Technology. Faculty of Information and Communication Technologies. Centre for Astrophysics and Supercomputing
- Source
- Monthly Notices of the Royal Astronomical Society, Vol. 356, no. 1 (2005), pp. 125-130
- Publication year
- 2005
- FOR Code(s)
- 0201 Astronomical and Space Sciences
- Publisher
- Blackwell
- ISSN
- 0035-8711
- Publisher URL
- http://dx.doi.org/10.1111/j.1365-2966.2004.08427.x
- Copyright
- Copyright © 2004 Royal Astronomical Society.
- Peer reviewed



