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Black Hole Spin Measurements in LMC X-1 and Cyg X-1 Are Highly Model Dependent
DOI: 10.3847/1538-4357/ad1b60 Bibcode: 2024ApJ...962..101Z

Zdziarski, Andrzej A.; Szanecki, Michał; Dewangan, Gulab +4 more

The black hole spin parameter, a *, was measured to be close to its maximum value of 1 in many accreting X-ray binaries. In particular, a * ≳ 0.9 was found in a number of studies of LMC X-1. These measurements were claimed to take into account both statistical and systematic uncertainties. We perform new measurements using a …

2024 The Astrophysical Journal
Suzaku 17
Discovery of a Second Eclipsing, ​​​​​Bursting Neutron Star Low-mass X-Ray Binary in the Globular Cluster Terzan 6
DOI: 10.3847/1538-4357/ad2f3d Bibcode: 2024ApJ...966..217V

Bahramian, Arash; Homan, Jeroen; Heinke, Craig O. +4 more

We have analyzed Chandra and Suzaku observations of the globular cluster Terzan 6, made when the recurrent transient GRS 1747–312 was in quiescence. Our analysis reveals the presence of a second eclipsing, bursting neutron star low-mass X-ray binary in the central regions of the cluster, in addition to GRS 1747–312. The new source, which we name T…

2024 The Astrophysical Journal
Gaia Suzaku eHST 4
Possible Supercritical Accretion on the Ultraluminous X-Ray Source in the Metal-poor Galaxy I Zw 18
DOI: 10.3847/1538-4357/ad4e34 Bibcode: 2024ApJ...970....8Y

Yoneyama, Tomokage; Matsumoto, Hironori; Noda, Hirofumi +2 more

We present an analysis of X-ray observations of the ultraluminous X-ray source (ULX) in I Zw 18 based on archival data taken with Chandra, XMM-Newton, and Suzaku. This ULX is considered to be an intermediate-mass black hole candidate simply because it is in the lowest-metallicity environment among ULXs, where the formation of heavy black holes is …

2024 The Astrophysical Journal
Suzaku XMM-Newton 0