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    The fading of two transient ultraluminous x-ray sources to below the stellar mass Eddington limit

    193418_193418.pdf (307.2Kb)
    Access Status
    Open access
    Authors
    Burke, M.
    Kraft, R.
    Soria, Roberto
    Maccarone, T.
    Raychaudhury, S.
    Sivakoff, G.
    Birkinshaw, M.
    Brassington, N.
    Forman, W.
    Hardcastle, M.
    Jones, C.
    Murray, S.
    Worrall, D.
    Date
    2013
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Burke, Mark J. and Kraft, Ralph P. and Soria, Roberto and Maccarone, Thomas J. and Raychaudhury, Somak and Sivakoff, Gregory R. and Birkinshaw, Mark and Brassington, Nicola J. and Forman, William R. and Hardcastle, Martin J. and Jones, Christine and Murray, Stephen S. and Worrall, Diana M. 2013. The fading of two transient ultraluminous x-ray sources to below the stellar mass Eddington limit. Astrophysical Journal. 775 (1): pp. 1-9.
    Source Title
    Astrophysical Journal
    DOI
    10.1088/0004-637X/775/1/21
    ISSN
    0004-637X
    Remarks

    This is an author-created, un-copy edited version of an article accepted for publication in the Astrophysical Journal. The publisher is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at http://doi.org/10.1088/0004-637X/775/1/21

    URI
    http://hdl.handle.net/20.500.11937/30082
    Collection
    • Curtin Research Publications
    Abstract

    We report new detections of the two transient ultraluminous X-ray sources (ULXs) in NGC 5128 from an ongoing series of Chandra observations. Both sources have previously been observed Lx (2-3) × ~1039 erg s–1, at the lower end of the ULX luminosity range. The new observations allow us to study these sources in the luminosity regime frequented by the Galactic black hole X-ray binaries (BH XBs). We present the recent lightcurves of both ULXs. 1RXH J132519.8-430312 (ULX1) was observed at Lx ≈ 1 × 1038 erg s–1, while CXOU J132518.2-430304 (ULX2) declined to Lx ≈ 2 × 1037 erg s–1 and then lingered at this luminosity for hundreds of days. We show that a reasonable upper limit for both duty cycles is 0.2, with a lower limit of 0.12 for ULX2. This duty cycle is larger than anticipated for transient ULXs in old stellar populations. By fitting simple spectral models in an observation with ~50 counts we recover properties consistent with Galactic BH XBs, but inconclusive as to the spectral state. We utilize quantile analyses to demonstrate that the spectra are generally soft, and that in one observation the spectrum of ULX2 is inconsistent with a canonical hard state at >95% confidence. This is contrary to what would be expected of an accreting intermediate mass black hole primary, which we would expect to be in the hard state at these luminosities. We discuss the paucity of transient ULXs discovered in early-type galaxies and excogitate explanations. We suggest that the number of transient ULXs scales with the giant and sub-giant populations, rather than the total number of XBs.

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