SIMBAD references

2015MNRAS.448.1153P - Mon. Not. R. Astron. Soc., 448, 1153-1161 (2015/April-1)

Spectral variability in Swift and Chandra observations of the ultraluminous source NGC 55 ULX1.

PINTORE F., ESPOSITO P., ZAMPIERI L., MOTTA S. and WOLTER A.

Abstract (from CDS):

NGC 55 ULX1 is a bright Ultraluminous X-ray source located 1.78 Mpc away. We analysed a sample of 20 Swift observations, taken between 2013 April and August, and two Chandra observations taken in 2001 September and 2004 June. We found only marginal hints of a limited number of dips in the light curve, previously reported to occur in this source, although the uncertainties due to the low counting statistics of the data are large. The Chandra and Swift spectra showed clearly spectral variability which resembles those observed in other ULXs. We can account for this spectral variability in terms of changes in both the normalization and intrinsic column density of a two-component model consisting of a blackbody (for the soft component) and a multicolour accretion disc (for the hard component). We discuss the possibility that strong outflows ejected by the disc are in part responsible for such spectral changes.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): accretion, accretion discs - galaxies: individual: NGC 55 - X-rays: binaries - X-rays: galaxies - X-rays: individuals: NGC 55 ULX1 - X-rays: individuals: XMMU J001528.9-391319

Simbad objects: 5

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2015MNRAS.448.1153P and select 'bookmark this link' or equivalent in the popup menu


2020.09.22-03:35:47

© Université de Strasbourg/CNRS

    • Contact