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  4. A Rapid Change in X-Ray Variability and a Jet Ejection in the Black Hole Transient MAXI J1820+070

A Rapid Change in X-Ray Variability and a Jet Ejection in the Black Hole Transient MAXI J1820+070

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sword-2020-10-30T16:22:03.original.xml (130 B)
Original SWORD entry document
Author(s)
Homan, Jeroen
•
Motta, Sara E.
•
Bright, Joe
•
Altamirano, Diego
•
Arzoumanian, Zaven
•
Basak, Arkadip
•
Belloni, Tomaso M.
•
Cackett, Edward M.
•
Fender, Rob
•
Gendreau, Keith C.
more
Date Issued
March 2020
Journal
Astrophysical Journal Letters
Publisher
American Astronomical Society
Citation
Homan, Jeroen et al. "A Rapid Change in X-Ray Variability and a Jet Ejection in the Black Hole Transient MAXI J1820+070." Astrophysical Journal Letters 891, 2 (March 2020): L29 © 2020 The American Astronomical Society
Version
Final published version
Abstract
We present Neutron Star Interior Composition Explorer X-ray and Arcminute Microkelvin Imager Large Array radio observations of a rapid hard-to-soft state transition in the black hole X-ray transient MAXI J1820+070. During the transition from the hard state to the soft state a switch between two particular types of quasiperiodic oscillations (QPOs) was seen in the X-ray power density spectra, from type-C to type-B, along with a drop in the strength of the broadband X-ray variability and a brief flare in the 7-12 keV band. Soon after this switch (∼2-2.5 hr) a strong radio flare was observed that corresponded to the launch of superluminal ejecta. Although hints of a connection between QPO transitions and radio flares have been seen in other black hole X-ray transients, our observations constitute the strongest observational evidence to date for a link between the appearance of type-B QPOs and the launch of discrete jet ejections.
MIT Department
MIT Kavli Institute for Astrophysics and Space Research
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
https://hdl.handle.net/1721.1/129585
DOI of Published Version
https://doi.org/10.3847/2041-8213/ab7932
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