Researchers using the Atacama Large Millimeter/submillimeter Array (ALMA) have found regions where certain organic molecules somehow endure the intense radiation near the supermassive black hole at the center of spiral galaxy M77, also known as NGC 1068.
To help understand why some galaxies “burst” while others do not, an international team of astronomers have dissected a cluster of star-forming clouds at the heart of NGC 253, one of the nearest starburst galaxies to the Milky Way.
Computer models suggest that dust grains grow when they collide and stick together. However, when these bigger grains collide again at high speed they are often smashed to pieces and sent back to square one.
With the help of ALMA (Atacama Large Millimeter/submillimeter Array), scientists have observed the "Subaru/XMM-Newton Deep Survey Field" in the direction of the constellation Cetus, and succeeded in identifying 15 dark galaxies.