Chadwick, P.M.; Chaty, S.; Daniel, M.K.; Haswell, C.A.; Kolb, U.; McComb, T.J.L.; McKenny, J.M.; Nolan, S.J.; Norton, A.J.; Orford, K.J.; Osborne, J.L. and Rayner, S.M.
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With new generation VHE telescopes, X-ray binary systems become very promising targets for VHE γ-ray observations. In particular, if sources with relativistic jets are thought of as galactic analogues of AGNs, the acceleration mechanisms should be similar. We survey the prospects of studying these objects with HESS, particularly in the context of multiwavelength studies.
|Item Type:||Journal Article|
|Academic Unit/Department:||Science > Physical Sciences|
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
|Depositing User:||Users 6827 not found.|
|Date Deposited:||04 Jul 2006|
|Last Modified:||05 Mar 2014 10:27|
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