paper

NuSTAR and Swift Observations of the Extragalactic Black Hole X-ray Binaries

arXiv:2108.10546 · doi:10.1093/mnras/stab2448

Abstract

We present the results obtained from detailed spectral and timing studies of extra-galactic black hole X-ray binaries LMC~X--1 and LMC~X--3, using simultaneous observations with {\it Nuclear Spectroscopic Telescope Array (NuSTAR)} and {\it Neil Gehrels Swift} observatories. The combined spectra in the ~keV energy range, obtained between 2014 and 2019, are investigated for both sources. We do not find any noticeable variability in ~keV light curves, with ~Hz fractional rms estimated to be \%. No evidence of quasi-periodic oscillations is found in the power density spectra. The sources are found to be in the high soft state during the observations with disc temperature ~keV, photon index, and thermal emission fraction, \%. An Fe K emission line is detected in the spectra of LMC~X--1, though no such feature is observed in the spectra of LMC~X--3. From the spectral modelling, the spins of the black holes in LMC~X--1 and LMC~X--3 are estimated to be in the range of and , respectively. The accretion efficiency is found to be, and for LMC~X--1 and LMC~X--3, respectively.

9 pages, 5 figures, accepted for publication in MNRAS. Comments are welcome

References in corpus (6)

Cited by in corpus (7)