An extremely powerful long-lived superluminal ejection from the black hole MAXI J1820+070
Accepted version
Peer-reviewed
Repository URI
Repository DOI
Change log
Authors
Abstract
Black holes in binary systems execute patterns of outburst activity where two
characteristic X-ray states are associated with different behaviours observed
at radio wavelengths. The hard state is associated with radio emission
indicative of a continuously replenished, collimated, relativistic jet, whereas
the soft state is rarely associated with radio emission, and never
continuously, implying the absence of a quasi-steady jet. Here we report radio
observations of the black hole transient MAXI J1820$+
Description
Keywords
Journal Title
Conference Name
Journal ISSN
2397-3366