Search Results - Black September
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Swift Observations of MAXI J1659-152: A Compact Binary with a Black Hole Accretor
Published 2011“…We report on the detection and follow-up high-cadence monitoring observations of MAXI J1659-152, a brightGalactic X-ray binary transient with a likely black hole accretor, by Swift over a 27 day period after its initialoutburst detection. …”
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An H i absorption distance to the black hole candidate X-ray binary MAXI J1535-571
Published 2019“…With the Australian Square Kilometre Array Pathfinder (ASKAP) we monitored the black hole candidate X-ray binary MAXI J1535-571 over seven epochs from 2017 September 21 to October 2. …”
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Combined analysis of Hubble and VLT photometry of the intermediate mass black hole ESO 243-49 HLX-1
Published 2013“…In this paper, we present a combined analysis of data obtained with the Hubble Space Telescope (HST), Very Large Telescope (VLT) and Swift X-ray telescope of the intermediate-mass black hole ESO 243−49 HLX-1 that were taken two months apart between 2010 September and November. …”
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Bright Mini-outburst Ends the 12 yr Long Activity of the Black Hole Candidate Swift J1753.5-0127
Published 2019“…We present optical, UV, and X-ray monitoring of the short orbital period black hole X-ray binary candidate Swift J1753.5-0127, focusing on the final stages of its 12 yr long outburst that started in 2005. …”
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Disk-Jet Coupling in the 2017/2018 Outburst of the Galactic Black Hole Candidate X-Ray Binary MAXI J1535-571
Published 2019“…MAXI J1535-571 is a Galactic black hole candidate X-ray binary that was discovered going into outburst in 2017 September. …”
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Broad-band monitoring tracing the evolution of the jet and disc in the black hole candidate X-ray binary MAXI J1659-152
Published 2013“…MAXI J1659-152 was discovered on 2010 September 25 as a new X-ray transient, initially identified as a gamma-ray burst, but was later shown to be a new X-ray binary with a black hole as the most likely compact object. …”
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Accretion states of the Galactic microquasar GRS 1758-258
Published 2011“…Our spectral and timing analysis of the XMM–Newton data shows that the source was in the canonical intermediate, soft and hard states in 2000 September 19, 2001 March 22 and 2002 September 28, respectively. …”
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Optical counterpart of HLX-1 during the 2010 outburst
Published 2012“…We conclude that during the 2010 September observations, the optical counterpart was dominated by emission from an irradiated disc (which responds to the varying X-ray luminosity), rather than by a star cluster around the black hole (which would not change). …”
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