Abstract
We have measured the Faraday rotation toward a large sample of polarized radio sources behind the Large Magellanic Cloud (LMC) to determine the structure of this galaxy's magnetic field. The magnetic field of the LMC consists of a coherent axisymmetric spiral of field strength similar to1 microgauss. Strong fluctuations in the magnetic field are also seen on small (
Original language | English |
---|---|
Pages (from-to) | 1610-1612 |
Journal | Science |
Volume | 307 |
DOIs | |
Publication status | Published - 2005 |