Ioannou, Zach; Haswell, C.; Hynes, R. ; Chaty, S.; Harlaftis, E.; Brinias, A.; Norton, A. J.; Fried, R.; Rolfe, D. and Solheim, J. E.
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We present optical and ifra-red photometry of the new X-ray transient source XTE J1859+226. The source exhibits a typical X-ray nova behaviour with a fast rise (~5 days) and an exponential decline (~23 days). Week photometric modulations are seen at several periods ranging from 9.15 hours to 20 minutes. The evolution of the spectral energy distribution of the source can be fitted very well with a model of an X-ray irradiated accretion disc.
|Item Type:||Conference Item|
|Copyright Holders:||2001 Hellenic Astronomical Society|
|Extra Information:||5th Hellenic Astronomical Conference, held 20-22 September, 2001 in Crete, Greece. Online at http://www.astro.auth.gr/elaset/helasmtg/2001/proceedings.htm, p.151.1|
|Academic Unit/School:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Andrew Norton|
|Date Deposited:||17 May 2011 08:12|
|Last Modified:||29 Nov 2016 14:16|
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