Jan 2, 2018 · The luminous X-ray binary 47 Tuc X9 shows radio and X-ray emission consistent with a stellar-mass black hole accreting from a carbon-oxygen white dwarf.
Dec 5, 2017 · The luminous X-ray binary 47 Tuc X9 shows radio and X-ray emission consistent with a stellar-mass black hole (BH) accreting from a carbon–oxygen white dwarf.
The luminous X-ray binary 47 Tuc X9 shows radio and X-ray emission consistent with a stellar-mass black hole accreting from a carbon-oxygen white dwarf.
The luminous X-ray binary 47 Tuc X9 shows radio and X-ray emission consistent with a stellar-mass black hole accreting from a carbon-oxygen white dwarf.
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47 Tuc X9 is easily the brightest X-ray source above 2 keV within the half-mass radius of 47 Tuc (Heinke et al. 2005b). The CV AKO 9 (Knigge et al. 2003) is the ...
The globular cluster (GC) 47 Tuc has recently been proposed to host an intermediate-mass black hole (IMBH) or a population of stellar mass black holes (BHs) ...
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.
Formation Constraints Indicate a Black Hole Accretor in 47 Tuc X9. Ross P. Church, Jay Strader, Melvyn B. Davies, Alexey Bobrick. https://doi.org/10.3847/2041 ...
Formation constraints indicate a black-hole accretor in 47 Tuc X9. Church, R ... No evidence for intermediate-mass black holes in globular clusters: Strong ...