SIMBAD references

2004MNRAS.351.1063S - Mon. Not. R. Astron. Soc., 351, 1063-1070 (2004/July-1)

A dipping black hole X-ray binary candidate in NGC 55.

STOBBART A.-M., ROBERTS T.P. and WARWICK R.S.

Abstract (from CDS):

XMM-Newton European Photon Imaging Camera (EPIC) observations have revealed a bright point-like X-ray source in the nearby Magellanic-type galaxy NGC 55. At the distance of NGC 55, the maximum observed X-ray luminosity of the source, designated as XMMU J001528.9-391319, is Lx∼ 1.6 x1039 erg/s, placing the object in the ultraluminous X-ray source (ULX) regime. The X-ray light curve exhibits a variety of features including a significant upward drift over the 60 ks observation. Most notably a series of X-ray dips are apparent with individual dips lasting for typically 100-300 s. Some of these dips reach almost 100 per cent diminution of the source flux in the 2.0-4.5 keV band. The EPIC CCD spectra can be modelled with two spectral components, a very soft power-law continuum (Γ ~ 4) dominant below 2 keV, plus a multicolour disc (MCD) component with an inner-disc temperature kT ~ 0.8 keV. The observed upward drift in the X-ray flux can be attributed to an increase in the level of the MCD component, whilst the normalization of the power-law continuum remains unchanged. The dipping episodes correspond to a loss of signal from both spectral components, although the blocking factor is at least a factor 2 higher for the MCD component. XMMU J001528.9-391319 can be considered as a candidate black hole binary (BHB) system. A plausible explanation of the observed temporal and spectral behaviour is that we view the accretion disc close to edge-on and that, during dips, orbiting clumps of obscuring material enter our line of sight and cause significant blocking or scattering of the hard thermal X-rays emitted from the inner disc. In contrast, the more extended source of the soft power-law flux is only partially covered by the obscuring matter during the dips.

Abstract Copyright: 2004 RAS

Journal keyword(s): accretion, accretion discs - X-rays: binaries - X-rays: galaxies

Simbad objects: 22

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2020.09.21-07:35:23

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