UV absorption toward 8 LMC stars shows redshifted gas near 30 Doradus that appears to trace the Magellanic arms B and E on the near side of the LMC, extending about 1 degree further than previously mapped.
A., Lehner , N., & Howk , J
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New Interpretation for the Orientation of the LMC's Gaseous Arms B and E using ULLYSES
UV absorption toward 8 LMC stars shows redshifted gas near 30 Doradus that appears to trace the Magellanic arms B and E on the near side of the LMC, extending about 1 degree further than previously mapped.