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dc.contributor.authorBahramian, A.
dc.contributor.authorHeinke, C.
dc.contributor.authorTudor, Vlad
dc.contributor.authorMiller-Jones, James
dc.contributor.authorBogdanov, S.
dc.contributor.authorMaccarone, T.
dc.contributor.authorKnigge, C.
dc.contributor.authorSivakoff, G.
dc.contributor.authorChomiuk, L.
dc.contributor.authorStrader, J.
dc.contributor.authorGarcia, J.
dc.contributor.authorKallman, T.
dc.identifier.citationBahramian, A. and Heinke, C. and Tudor, V. and Miller-Jones, J. and Bogdanov, S. and Maccarone, T. and Knigge, C. et al. 2017. The ultracompact nature of the black hole candidate X-ray binary 47 Tuc X9. Monthly Notices of the Royal Astronomical Society. 467 (2): pp. 2199-2216.

47 Tuc X9 is a low-mass X-ray binary (LMXB) in the globular cluster 47 Tucanae, and was previously thought to be a cataclysmic variable. However, Miller-Jones et al. recently identified a radio counterpart to X9 (inferring a radio/X-ray luminosity ratio consistent with black hole LMXBs), and suggested that the donor star might be a white dwarf. We report simultaneous observations of X9 performed by Chandra, NuSTAR and Australia Telescope Compact Array. We find a clear 28.18 ± 0.02-min periodic modulation in the Chandra data, which we identify as the orbital period, confirming this system as an ultracompact X-ray binary. Our X-ray spectral fitting provides evidence for photoionized gas having a high oxygen abundance in this system, which indicates a C/O white dwarf donor. We also identify reflection features in the hard X-ray spectrum, making X9 the faintest LMXB to show X-ray reflection. We detect an ~6.8-d modulation in the X-ray brightness by a factor of 10, in archival Chandra, Swiftand ROSAT data. The simultaneous radio/X-ray flux ratio is consistent with either a black hole primary or a neutron star primary, if the neutron star is a transitional millisecond pulsar. Considering the measured orbital period (with other evidence of a white dwarf donor), and the lack of transitional millisecond pulsar features in the X-ray light curve, we suggest that this could be the first ultracompact black hole X-ray binary identified in our Galaxy.

dc.publisherOxford University Press
dc.titleThe ultracompact nature of the black hole candidate X-ray binary 47 Tuc X9
dc.typeJournal Article
dcterms.source.titleMonthly Notices of the Royal Astronomical Society

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusOpen access

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