️<unk>️<unk>️<unk>️  ️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️ ️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️ ️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️ <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> ️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️ Blue objects are radio galaxies with streams of plasma, and in green is the 'Large Relic', which could be a shockwave as the clusters collide.<unk> Blue objects are radio galaxies with streams of plasma, and in green is the 'Large Relic', which could be a shockwave as the clusters collide. Researchers at the National Radio Astronomy Observatory (NRAO) made the image using the Karl G. Jansky Very Large Array (VLA) in New Mexico.<unk> Researchers at the National Radio Astronomy Observatory (NRAO) made the image using the Karl G. Jansky Very Large Array (VLA) in New Mexico. In the image, red coloration shows longer radio waves, moving down to blue, which is composed of shorter radio waves.<unk> In the image, red coloration shows longer radio waves, moving down to blue, which is composed of shorter radio waves. region is known as Abell 2256, and is about 800 million light-years from Earth and about four million light-years across.<unk> region is known as Abell 2256, and is about 800 million light-years from Earth and about four million light-years across. The image covers an area in the sky almost as large as the full moon.<unk> The image covers an area in the sky almost as large as the full moon. ️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️ ️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️ ️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️ Radio galaxies can be detected at great distances, which makes then useful tools in studying the structure of the universe.<unk> Radio galaxies can be detected at great distances, which makes then useful tools in studying the structure of the universe.<unk> Radio galaxies can be detected at great distances, which makes then useful tools in studying the structure of the universe. Star formation in such galaxies is a strong source of radio waves, which come from supernova remnants and cosmic rays that are energized in the star formation regions.<unk> ️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️ In clusters like this the unusual shapes of the radio galaxies are due to the interaction of those jets with the cluster...
<unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> <unk> The'true color'image shows how radio waves would look to humans.<unk> The'true color'image shows how radio waves would look to humans.<unk> <unk> <unk> <unk> <unk> ️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️<unk>️