Disk, corona, jet connection in the intermediate state of MAXI J1820+070 revealed by NICER spectral-timing analysis

Journal article

We analyze five epochs of Neutron star Interior Composition Explorer (NICER) data of the black hole X-ray binary MAXI J1820+070 during the bright hard-to-soft state transition in its 2018 outburst with both reflection spectroscopy and Fourier-resolved timing analysis. We confirm the previous discovery of reverberation lags in the hard state, and find that the frequency range where the (soft) reverberation lag dominates decreases with the reverberation lag amplitude increasing during the transition, suggesting an increasing X-ray emitting region, possibly due to an expanding corona. By jointly fitting the lag-energy spectra in a number of broad frequency ranges with the reverberation model reltrans, we find the increase in reverberation lag is best described by an increase in the X-ray coronal height. This result, along with the finding that the corona contracts in the hard state, suggests a close relationship between spatial extent of the X-ray corona and the radio jet. We find the corona expansion (as probed by reverberation) precedes a radio flare by ∼5 days, which may suggest that the hard-to-soft transition is marked by the corona expanding vertically and launching a jet knot that propagates along the jet stream at relativistic velocities.

Authors: Wang, J; Mastroserio, G; Kara, E; Garcia, JA; Ingram, A

• Publication status: Published
• Peer review status: Peer reviewed
• Publisher: IOP Science
• Journal: Astrophysical Journal Letters
• Volume: 910
• Issue: 1
• Article number: L3
• Publication date: 2021-03-19
• Acceptance date: 2021-03-07
• DOI: 10.3847/2041-8213/abec79
• EISSN: 2041-8213
• ISSN: 2041-8205
• Language: English
• Keywords: black hole physics; high energy astrophysics; x-ray transient sources; stellar mass black holes; low-mass x-ray binary stars