Extragalactic Hot Molecular Core (2 of 2) (IMAGE) Tohoku University Caption Fig.2) Left: Distributions of molecular line emission from a hot molecular core in the Large Magellanic Cloud observed with ALMA. Emissions from dust, sulfur dioxide (SO2), nitric oxide (NO), and formaldehyde (H2CO) are shown as examples. Right: An infrared image of the surrounding star-forming region (based on the 8 micron data provided by the NASA/Spitzer Space Telescope). Credit T. Shimonishi/Tohoku University, ALMA (ESO/NAOJ/NRAO) Usage Restrictions Credit: T. Shimonishi/Tohoku University, ALMA (ESO/NAOJ/NRAO) License Licensed content Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.