Proper Motion and Natal Kick in the Galactic Black Hole X-Ray Binary AT2019wey

• Published in: The Astrophysical journal Vol. 983; no. 2; pp. 147 - 152
• Main Authors: Cui, Lang, Jiang, Pengfei, An, Tao, Cao, Hongmin, Chang, Ning, Migliori, Giulia, Giroletti, Marcello, Frey, Sándor, Yang, Jun, Gabányi, Krisztina É., Hong, Xiaoyu, Zhang, Wenda
• Format: Journal Article
• Language: English
• Published: The American Astronomical Society 20.04.2025; IOP Publishing
• Subjects: Proper motions; Stellar mass black holes; Very long baseline interferometry; X-ray binary stars
• ISSN: 0004-637X; 1538-4357; 1538-4357
• DOI: 10.3847/1538-4357/adc0f7

Understanding the formation mechanisms of stellar-mass black hole X-ray binaries (BHXBs) remains a fundamental challenge in astrophysics. The natal kick velocities imparted during black hole (BH) formation provide crucial constraints on these formation channels. In this work, we present a new-epoch very long baseline interferometry (VLBI) observation of the Galactic BHXB AT2019wey carried out in 2023. Combining with archival VLBI data from 2020, we successfully measure the proper motion of AT2019wey over a 3 yr timescale, namely, 0.78 ± 0.12 mas yr −1 in R.A. and −0.42 ± 0.07 mas yr −1 in decl. Employing the measured proper motion, we estimate its peculiar velocity and the potential kick velocity (PKV) through Monte Carlo simulations, incorporating uncertainties of its distance and radial velocity. The estimated PKV distributions and height above the Galactic plane suggest that AT2019wey’s BH likely formed through a supernova explosion rather than direct collapse.