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SUMMARY:Investigating Relativistic Jets in X-ray Binaries through Multi-Wa
 velength Timing Studies
DTSTART;VALUE=DATE-TIME:20261028T180500Z
DTEND;VALUE=DATE-TIME:20261028T181500Z
DTSTAMP;VALUE=DATE-TIME:20261026T232643Z
UID:indico-contribution-3628@nyx.physics.mcgill.ca
DESCRIPTION:Speakers: Élodie Lescure (University of Lethbridge)\nRelativi
 stic jets launched from accreting compact objects are thought to play an i
 mportant role in the Universe\, influencing large-scale processes such as 
 galaxy evolution and star formation. However\, the connection between thei
 r properties and those of the accretion flow remains poorly understood. Mu
 lti-wavelength time-domain observations of black hole X-ray binaries provi
 de a new avenue to study this connection in detail. By probing different c
 omponents of the system at different wavelengths\, these observations allo
 w us to trace the evolution of gas from inflow to outflow. Recently\, we l
 aunched a first-of-its-kind observational program designed to obtain multi
 -wavelength time-domain observations spanning an entire X-ray binary outbu
 rst. In this talk\, I will present the first results from this program\, i
 ncluding recent ALMA and VLT observations of BW Cir (GS 1354-64).\n\nhttps
 ://nyx.physics.mcgill.ca/event/587/contributions/3628/
LOCATION:Online 
URL:https://nyx.physics.mcgill.ca/event/587/contributions/3628/
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