Different line-of-sight velocities of the molecular gas around LL Pegasi

Visualizing the ALMA image cube of LL Pegasi

Visualizing the ALMA image cube of LL Pegasi. Each frame of the video shows the molecular gas material surrounding LL Pegasi for a different line-of-sight velocity. This velocity, advancing 1 km/s per frame, is given at the top-right corner. The field size is 20,000 times the distance between the Sun and the Earth.

Supernova 1987A
Artist's impression of Supernova 1987A
Phoenix Cluster

ALMA Discovers Unexpected Trove of Star-forming Gas in Phoenix Cluster

Video explaining the complex relationship between a supermassive black hole and its host galaxy in the Phoenix Cluster, as studied with ALMA. Jets from the black hole create giant radio bubbles. Hugging these bubbles are filaments of cold, dense gas that could eventually fuel future star formation and feed the galaxy’s active supermassive black hole.

Artist's impression of 3C 120

Animation of a Black Hole

Artist’s conception of region near the supermassive black hole inside the radio galaxy known as 3C 120, where twisted magnetic fields propel and shape jets of particles.