![]() ![]() ![]() This fades and becomes resolved out after 4 days, after which a second component appears to the north, moving in the opposite direction. We initially see only the southern component, whose evolution gives rise to a 15-mJy radio flare and generates the observed radio polarization. We show that following a hard-to-soft state transition, we detect moving jet knots that appear asymmetric in morphology and brightness, and expand to become laterally resolved as they move away from the core, along an axis aligned approximately -11° east of north. ![]() Here we report high angular resolution radio observations of the 2013 outburst of the black hole candidate X-ray binary system XTE J1908+094, using data from the Very Long Baseline Array and European VLBI Network. Tudose, V.īlack hole X-ray binaries undergo occasional outbursts caused by changing inner accretion flows. ![]() Resolved, expanding jets in the Galactic black hole candidate XTE J1908+094 ![]()
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