Sutaria, F. K.; Kolb, U.; Charles, P.; Osborne, J. P.; Kuulkers, E.; Casares, J.; Harlaftis, E. T.; Shahbaz, T.; Still, M. and Wheatley, P.
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|DOI (Digital Object Identifier) Link:||http://doi.org/10.1051/0004-6361:20020842|
|Google Scholar:||Look up in Google Scholar|
The soft X-ray transient GU Mus has been detected by XMM-Newton in the quiescent state. The source is very faint, with a 0.5-10.0 keV unabsorbed flux of ≃ 1.1 x 10-14 ergs cm-2 s-1. The spectra is well fit by an absorbed powerlaw with a photon index of α = 1.6 ± 0.4, close to the value seen when the source was in the low/hard state in Aug. 1991. From our observed luminosity, it seems unlikely that the quiescent state emission is dominated by coronal X-rays from the secondary. The flux also appears to be in agreement with the ADAF model of BH-transients in quiescence.
|Item Type:||Journal Article|
|Copyright Holders:||2002 ESO|
|Keywords:||binary X-rays; GU Mus; black hole physics; accretion; accretion disks|
|Academic Unit/Department:||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:||Users 6827 not found.|
|Date Deposited:||06 Jul 2006|
|Last Modified:||05 Oct 2016 02:46|
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