HI4PI Animation (VIDEO) International Centre for Radio Astronomy Research This video is under embargo. Please login to access this video. To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video Caption Using real data, this animation shows radio emission from neutral hydrogen atoms located in our galaxy, the Milky Way, and our neighboring dwarf galaxies, the Large and Small Magellanic Clouds. It has been produced using observations made with the 100 meter Max-Planck radio telescope in Effelsberg, Germany, and the 64 meter CSIRO radio telescope in Parkes, Australia. The colors reflect the approaching (purple/blue) and receding (orange/green)hydrogen gas motion while the brightness traces its amount. Credit Credit: Lister Staveley-Smith, Benjamin Winkel and the HI4PI collaboration. Usage Restrictions Attribution 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.