SIMBAD references

2011MNRAS.414L.104D - Mon. Not. R. Astron. Soc., 414, L104-L108 (2011/June-2)

Swift detection of an intermediately long X-ray burst from the very faint X-ray binary XMMU J174716.1–281048.

DEGENAAR N., WIJNANDS R. and KAUR R.

Abstract (from CDS):

We report on the Swift detection of a thermonuclear X-ray burst from the very-faint quasi-persistent neutron star X-ray binary XMMU J174716.1–281048, which triggered the satellite's Burst Alert Telescope (BAT) on 2010 August 13. Analysis of the BAT spectrum yields an observed bolometric peak flux of ≃ 4.5 {x} 10–8 erg/cm2/s, from which we infer a source distance of ≲ 8.4 kpc. Follow-up observations with Swift's X-ray Telescope (XRT) suggest that the event had a duration of ≃ 3 h and a total radiated energy of ≃ 9 {x} 1040 erg, which classify it as an intermediately long X-ray burst. This is only the second X-ray burst ever reported from this source. Inspection of Swift/XRT observations performed between 2007 and 2010 suggests that the 2–10 keV accretion luminosity of the system is ≃ 5 {x} 1034 erg/s for an assumed distance of 8.4 kpc. Despite being transient, XMMU J174716.1–281048 appears to have been continuously active since its discovery in 2003.

Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS

Journal keyword(s): accretion, accretion discs - stars: neutron - X-rays: binaries - X-rays: bursts - Xrays: individual (XMMU J174716.1-281048, IGR J17464-2811)

Simbad objects: 5

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2020.09.28-18:10:44

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