We use data from the bright atoll source 4U 1705-44 taken with XMM-Newton, BeppoSAX, and RXTE both in the hard and in the soft state to perform a self-consistent study of the reflection component in this source. Although the data from these X-ray observatories are not simultaneous, the spectral decomposition is shown to be consistent among the different observations, when the source flux is similar. We have therefore selected observations performed at similar flux levels in the hard and soft states to study the spectral shape in these two states in a broad-band (0.1-200 keV) energy range, with good energy resolution, and using self-consistent reflection models. These reflection models provide a good fit for the X-ray spectrum both in the hard and in the soft state in the whole spectral range. We discuss the differences in the main spectral parameters we find in both states, providing evidence that the inner radius of the optically thick disk slightly recedes in the hard state.

Egron, E., Di Salvo, T., Motta, S., Burderi, L., Papitto, A., Duro, R., et al. (2013). Testing reflection features in 4U 1705-44 with XMM-Newton, BeppoSAX, and RXTE in the hard and soft states. ASTRONOMY & ASTROPHYSICS, 550, 5 [10.1051/0004-6361/201219675].

Testing reflection features in 4U 1705-44 with XMM-Newton, BeppoSAX, and RXTE in the hard and soft states

DI SALVO, Tiziana;D'AI', Antonino;IARIA, Rosario;
2013

Abstract

We use data from the bright atoll source 4U 1705-44 taken with XMM-Newton, BeppoSAX, and RXTE both in the hard and in the soft state to perform a self-consistent study of the reflection component in this source. Although the data from these X-ray observatories are not simultaneous, the spectral decomposition is shown to be consistent among the different observations, when the source flux is similar. We have therefore selected observations performed at similar flux levels in the hard and soft states to study the spectral shape in these two states in a broad-band (0.1-200 keV) energy range, with good energy resolution, and using self-consistent reflection models. These reflection models provide a good fit for the X-ray spectrum both in the hard and in the soft state in the whole spectral range. We discuss the differences in the main spectral parameters we find in both states, providing evidence that the inner radius of the optically thick disk slightly recedes in the hard state.
Settore FIS/05 - Astronomia E Astrofisica
http://adsabs.harvard.edu/abs/2013A%26A...550A...5E
Egron, E., Di Salvo, T., Motta, S., Burderi, L., Papitto, A., Duro, R., et al. (2013). Testing reflection features in 4U 1705-44 with XMM-Newton, BeppoSAX, and RXTE in the hard and soft states. ASTRONOMY & ASTROPHYSICS, 550, 5 [10.1051/0004-6361/201219675].
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/10447/73488
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