![Left: RGB image of 30 Dor for [C ii] with blue, 235–245 km s−1; green, 245–255 km s−1; and red, 255–270 km s−1. The contours indicate the HAWC+ 214 μm dust continuum emission starting at 0.1 Jy pixel−1 with increments of 0.1 Jy pixel−1. The yellow cross is added to guide the eye at the axes of what appears to be dominantly blueshifted and redshifted gas. The white segments indicate the magnetic field morphology on the RGB image. Right: the same for 12CO(2-1). -- USRA/Astrophysical Journal](https://i0.wp.com/spacenews.com/wp-content/uploads/2023/06/despite.png?resize=1200%2C722&ssl=1)
New research from the Stratospheric Observatory for Infrared Astronomy (SOFIA), whose science mission operations were managed by Universities Space Research Association, has shown that the magnetic fields in 30 Doradus […]
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