XMM-NewtonandSwiftobservations of XTE J1743-363
نویسندگان
چکیده
منابع مشابه
Xmm-newton Observations of Xte J1817-330 and Xte J1856+053
The black hole candidate XTE J1817-330 was discovered in outburst on 26 January 2006 with RXTE/ASM. One year later, on 28 February 2007, another X-ray transient discovered in 1996, XTE J1856+053, was detected by RXTE during a new outburst. We report on the spectra obtained by XMM-Newton of these two black hole candidates.
متن کاملLooking for black-holes in X-ray binaries with XMM-Newton: XTE J1817-330 and XTE J1856+053
The X-ray binary XTE J1817-330 was discovered in outburst on 26 January 2006 with RXTE/ASM. One year later, another X-ray transient discovered in 1996, XTE J1856+053, was detected by RXTE during a new outburst on 28 February 2007. We triggered XMM-Newton target of opportunity observations on these two objects to constrain their parameters and search for a stellar black holes. We summarize the p...
متن کاملXmm-newton Observation of the 5.25 Ms Transient Millisecond Pulsar Xte J1807–294 in Outburst
We report on the results obtained for the millisecond transient X–ray pulsar XTE J1807–294 in a 40 min orbital period system, based on an XMM-Newton ToO observation carried out during March 2003. The source was found at a luminosity level of about 2× 10 erg s in the 0.5–10 keV range (assuming a distance of 8 kpc). We confirm the presence of the 5.25 ms pulsations (after accounting for the orbit...
متن کاملXMM–Newton observations of the black hole X-ray transient XTE J1650–500 in quiescence
We report the result of an XMM–Newton observation of the black hole X-ray transient XTE J1650–500 in quiescence. The source was not detected, and we set upper limits on the 0.5–10 keV luminosity of 0.9–1.0 × 1031 erg s−1 (for a newly derived distance of 2.6 kpc). These limits are in line with the quiescent luminosities of black hole X-ray binaries with similar orbital periods (∼7–8 h).
متن کاملXmm-newton Spectroscopy of the Accretion-driven Millisecond X-ray Pulsar Xte J1751-305 in Outburst
We present an analysis of the first high-resolution spectra measured from an accretion-driven millisecond Xray pulsar in outburst. We observed XTE J1751–305 with XMM-Newton on 2002 April 7 for approximately 35 ks. Using a simple absorbed blackbody plus power-law model, we measure an unabsorbed flux of 6.6± 0.1× 10−10 erg cm−2 s−1 (0.5–10.0 keV). A hard power-law component (Γ = 1.44± 0.01) contr...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2013
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/201321248