The nucleus of the Milky Way is known to harbour regions of intense star formation activity as well as a supermassive black hole1. Recent observations have revealed regions of γ-ray emission reaching far above and below the Galactic Centre (relative to the Galactic plane), the so-called ‘Fermi bubbles’2. It is uncertain whether these were generated by nuclear star formation or by quasar-like outbursts of the central black hole3,4,5,6 and no information on the structures’ magnetic field has been reported. Here we report observations of two giant, linearly polarized radio lobes, containing three ridge-like substructures, emanating from the Galactic Centre. The lobes each extend about 60 degrees in the Galactic bulge, closely corresponding to the Fermi bubbles, and are permeated by strong magnetic fields of up to 15 microgauss. We conclude that the radio lobes originate in a biconical, star-formation-driven (rather than black-hole-driven) outflow from the Galaxy’s central 200 parsecs that transports a huge amount of magnetic energy, about 1055 ergs, into the Galactic halo. The ridges wind around this outflow and, we suggest, constitute a ‘phonographic’ record of nuclear star formation activity over at least ten million years.
Access optionsAccess options
Subscribe to Journal
Get full journal access for 1 year
only $3.90 per issue
All prices are NET prices.
VAT will be added later in the checkout.
Rent or Buy article
Get time limited or full article access on ReadCube.
All prices are NET prices.
This work has been carried out in the framework of the S-band Polarization All Sky Survey collaboration (S-PASS). We thank the Parkes Telescope staff for support, both while setting up the non-standard observing mode and during the observing runs. R.M.C. thanks F. Aharonian, R. Beck, G. Bicknell, D. Jones, C. Law, M. Morris, C. Pfrommer, W. Reich, A. Stolte, T. Porter and H. Völk for discussions, and the Max-Planck-Institut für Kernphysik for supporting his research. R.M.C. also acknowledges the support of a Future Fellowship from the Australian Research Council through grant FT110100108. B.M.G. and C.P. acknowledge the support of an Australian Laureate Fellowship from the Australian Research Council through grant FL100100114. M.H. acknowledges the support of research programme 639.042.915, which is partly financed by the Netherlands Organisation for Scientific Research (NWO). The Parkes Radio Telescope is part of the Australia Telescope National Facility, which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. We acknowledge the use of WMAP data and the HEALPix software package.
This file contains Supplementary Text and Data 1-9, Supplementary Tables 1-3, additional references and Supplementary Figures 1-6.
About this article