NICER observations of the black hole candidate MAXI J0637430 during the 2019-2020 Outburst
arXiv:2104.13005 · doi:10.1093/mnras/stab1231
Abstract
We present detailed timing and spectral studies of the black hole candidate MAXI J0637430 during its 2019-2020 outburst using observations with the {\em Neutron Star Interior Composition Explorer (NICER)} and the {\em Neil Gehrels Swift Observatory}. We find that the source evolves through the soft-intermediate, high-soft, hard-intermediate and low-hard states during the outburst. No evidence of quasi-periodic oscillations is found in the power density spectra of the source. Weak variability with fractional rms amplitude is found in the softer spectral states. In the hard-intermediate and hard states, high variability with the fractional rms amplitude of is observed. The keV spectra with {\em NICER} are studied with a combined disk-blackbody and nthcomp model along with the interstellar absorption. The temperature of the disc is estimated to be keV in the rising phase and decreased slowly to keV in the declining phase. The disc component was not detectable or absent during the low hard state. From the state-transition luminosity and the inner edge of the accretion flow, we estimate the mass of the black hole to be in the range of 512 , assuming the source distance of kpc.
14 pages, 11 figures, 1 table. Accepted for publication in MNRAS
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- Global Accretion Properties of Black Hole X-Ray Binaries: A Phenomenological Perspective
- Broadband X-ray Spectroscopy and Estimation of Spin of the Galactic Black Hole Candidate GRS 1758-258
- Spectral properties of soft X-ray transient MAXI J0637430 using AstroSat
- The spin measurement of MAXI J0637-430: a black hole candidate with high disk density
- Spectral and Timing Analysis of NuSTAR and Swift/XRT Observations of the X-Ray Transient MAXI J0637-430