The fading of two transient ULXs to below the stellar mass Eddington limit
arXiv:1307.8157 · doi:10.1088/0004-637X/775/1/21
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)E39 erg/s, 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 ~ 1E38 erg/s, while CXOU J132518.2-430304 (ULX2) declined to Lx ~ 2E37 erg/s 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 utilise 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 IMBH 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.
Accepted for publication in ApJ, 9 pages, 4 figures, 3 tables
References in corpus (11)
- X-ray Properties of Black-Hole Binaries
- X-ray observations of ultraluminous X-ray sources
- The hard X-ray spectral evolution in X-ray binaries and its application to constrain the black hole mass of ultraluminous X-ray sources
- The Discovery of Cepheids and a Distance to NGC 5128
- Orbital Period and Outburst Luminosity of Transient Low Mass X-ray Binaries
- Low-Mass X-ray Binaries and Globular Clusters in Centaurus A
- Deep Chandra Monitoring Observations of NGC 3379: Catalog of Source Properties
- A Transient Black-Hole Low-Mass X-Ray Binary Candidate in Centaurus A
- Discovery of a Highly Variable Dipping Ultraluminous X-ray source in M94
- The Remarkable Stability of Probable Black Hole Low-Mass X-ray Binaries in Nearby Galaxies
- Super-Eddington Accretion in the Ultraluminous X-ray Source NGC1313 X-2: An Ephemeral Feast
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- A Long-term Study of Ultraluminous X-ray Sources in NGC 891
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