Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 407, Issue 1, Pages 645-650Publisher
WILEY-BLACKWELL
DOI: 10.1111/j.1365-2966.2010.16943.x
Keywords
galaxies: individual: SDSS J122518; 86+144547; 7; X-rays: binaries; X-rays: individual: CXO J122518; 6+144545
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Funding
- Netherlands Organisation for Scientific Research
- Science and Technology Facilities Council [ST/H00243X/1] Funding Source: researchfish
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In this paper we report the discovery of CXO J122518.6+144545, a peculiar X-ray source with a position 3.6 +/- 0.2 arcsec off-nuclear from a Sloan Digital Sky Survey Data Release 7 (SDSS DR7) z = 0.0447 galaxy. The 3.6 arcsec offset corresponds to 3.2 kpc at the distance of the galaxy. The 0.3-8 keV X-ray flux of this source is 5 x 10-14 erg cm-2 s-1 and its 0.3-8 keV luminosity is 2.2 x 1041 erg s-1 (2.7 x 1041 erg s-1; 0.5-10 keV) assuming that the source belongs to the associated galaxy. We find a candidate optical counterpart in archival Hubble Space Telescope/Advanced Camera for Surveys g'-band observations of the field containing the galaxy obtained on 2003 June 16. The observed magnitude of g' = 26.4 +/- 0.1 corresponds to an absolute magnitude of -10.1. We discuss the possible nature of the X-ray source and its associated candidate optical counterpart and conclude that the source is either a very blue Type IIn supernova, an ultraluminous X-ray source with a very bright optical counterpart or a recoiling supermassive black hole.
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