The Cigar Galaxy is the archetypal starburst galaxy, having experienced two recent spates of star formation. One occurred10 million years ago in its nucleus, and another sprang up 5 million years ago in a ring around the galaxy’s core. This froth of starbirth drives a so-called galactic superwind: dust, gas, and radiation that flow out of the galaxy and into intergalactic space.

To observe this wind, Terry Jay Jones (University of Minnesota) and colleagues applied for time on NASA’s SOFIA airborne observatory, which soars above much of the atmosphere that would absorb the infrared light it’s designed to collect. A modified Boeing 747 flies the 2.7-meter telescope in whatever careening trajectories are necessary to best view its targets that night.

Jones and colleagues used the High-resolution Airborne Wideband Camera-plus (HAWC+) instrument aboard SOFIA to observe far-infrared light (at wavelengths of 53 and 154 microns) coming from the Cigar Galaxy. Hot dust within giant, gaseous star-factory clouds emits this light. But dust isn’t perfectly spherical; dust grains tend to be oblong, and they tend to align with the ambient magnetic field that threads the galaxy. So the emission from these dust grains is polarized in a way that tells astronomers which way the magnetic field is pointing.

What Jones’s team found was that within 2,000 light-years of the galaxy’s center, the wind that charges into intergalactic space carries the galaxy’s magnetic field along with it. The polarization in the image above shows that the magnetic field is pretty much vertical in this central region. Outside this region, the magnetic field is horizontal, threading the plane of the galaxy.