The Ejection of Transient Jets in Swift J1727.8−1613 Revealed by Time-dependent Visibility Modeling

The Ejection of Transient Jets in Swift J1727.8−1613 Revealed by Time-dependent Visibility Modeling

High angular resolution radio observations of relativistic jets are necessary to understand the causal connection between accretion and jet ejection in low-mass X-ray binaries. Images from these observations can be difficult to reconstruct due to the rapid intra-observational motion and variability...

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Bibliographic Details
Main Authors: Callan M. Wood, James C. A. Miller-Jones, Arash Bahramian, Steven J. Tingay, He-Xin Liu, Diego Altamirano, Rob Fender, Elmar Körding, Dipankar Maitra, Sera Markoff, David M. Russell, Thomas D. Russell, Craig L. Sarazin, Gregory R. Sivakoff, Roberto Soria, Alexandra J. Tetarenko, Valeriu Tudose
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
Stellar mass black holes
Radio jets
Relativistic jets
Very long baseline interferometry
Low-mass x-ray binary stars
Transient sources
Online Access:https://doi.org/10.3847/2041-8213/adc9b3
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https://doi.org/10.3847/2041-8213/adc9b3

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