Figure-01-01-01-01.png
Figure 1. Left: Global 3.5mm VLBI image down to 37 microarcseconds (hyper-) resolution, including the VLBA, GBT, and ALMA, of the SMBH and jet in M87 from scales of a few gravitational radii to a few parsec (Lu et al. 2023, Nature, 616, 686). Right: VLBA 43 GHz observations showing jet precession with an 11 year period (Cui et al. 2023, Nature, 621, 711).
https://science.nrao.edu/science/highlights/images/2023/Figure-01-01-01-01.png/view
https://science.nrao.edu/science/highlights/images/2023/Figure-01-01-01-01.png/@@download/image/Figure-01-01-01-01.png
Figure-01-01-01-01.png
Figure 1. Left: Global 3.5mm VLBI image down to 37 microarcseconds (hyper-) resolution, including the VLBA, GBT, and ALMA, of the SMBH and jet in M87 from scales of a few gravitational radii to a few parsec (Lu et al. 2023, Nature, 616, 686). Right: VLBA 43 GHz observations showing jet precession with an 11 year period (Cui et al. 2023, Nature, 621, 711).
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