Discovery of a Highly Variable Dipping Ultraluminous X-Ray Source in M94

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dc.contributor.author Lin, Dacheng
dc.contributor.author Irwin, Jimmy A.
dc.contributor.author Webb, Natalie A.
dc.contributor.author Didier, Barret
dc.contributor.author Remillard, Ronald A.
dc.date.accessioned 2018-09-12T19:38:48Z
dc.date.available 2018-09-12T19:38:48Z
dc.date.issued 2013-12-20
dc.identifier.citation Lin, D., Irwin, J., Webb, N., Barret, D., Remillard, R. (2013): Discovery of a Highly Variable Dipping Ultraluminous X-Ray Source in M94. The Astrophysical Journal, 779(2). en_US
dc.identifier.uri http://ir.ua.edu/handle/123456789/3841
dc.description.abstract We report the discovery of a new ultraluminous X-ray source (ULX) 2XMM J125048.6+410743 within the spiral galaxy M94. The source has been observed by ROSAT, Chandra, and XMM-Newton on several occasions, exhibiting as a highly variable persistent source or a recurrent transient with a flux variation factor of 100, a high duty cycle (at least ∼70%), and a peak luminosity of LX ∼ 2 × 1039 erg s−1 (0.2–10 keV, absorbed). In the brightest observation, the source is similar to typical low-luminosity ULXs, with the spectrum showing a high-energy cutoff but harder than that from a standard accretion disk. There are also sporadical short dips, accompanied by spectral softening. In a fainter observation with LX ∼ 3.6×1038 erg s−1, the source appears softer and is probably in the thermal state seen in Galactic black hole X-ray binaries (BHBs). In an even fainter observation (LX ∼ 9×1037 erg s−1), the spectrum is harder again, and the source might be in the steep-power-law state or the hard state of BHBs. In this observation, the light curve might exhibit ∼7 hr (quasi-)periodic large modulations over two cycles. The source also has a possible point-like optical counterpart from Hubble Space Telescope images. In terms of the colors and the luminosity, the counterpart is probably a G8 supergiant or a compact red globular cluster containing ∼2 × 105 K dwarfs, with some possible weak UV excess that might be ascribed to accretion activity. Thus, our source is a candidate stellar-mass BHB with a supergiant companion or with a dwarf companion residing in a globular cluster. Our study supports that some low-luminosity ULXs are supercritically accreting stellar-mass BHBs. en_US
dc.format.mimetype application/pdf en_US
dc.subject accretion, accretion disks en_US
dc.subject black hole physics en_US
dc.subject X-rays: binaries en_US
dc.subject X-rays: individual: 2XMM J125048.6+410743 en_US
dc.title Discovery of a Highly Variable Dipping Ultraluminous X-Ray Source in M94 en_US
dc.type text en_US


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