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This animated gif shows the structure and motions (speed in direction towards the Sun) of gas in the forming cluster, as seen with ALMA (purple) on top of the infrared Hubble image. The color-scales from pink-purple to blue-purple represent the gas moving at different velocities, from 15km/s to 24 km/s. These motions are controlled by gravity, turbulence and wind and radiation pressure “feedback” from the new-born stars.
ALMA Mosaic Star Cluster (animated gif)more_horiz
Image of star cluster G286.21+0.17, caught in the act of formation. This is a multiwavelength mosaic of more than 750 ALMA radio images, and 9 Hubble infrared images. ALMA shows molecular clouds (purple) and Hubble shows stars and glowing dust (yellow and red).
ALMA Mosaic Star Clustermore_horiz
WLM dwarf irregular galaxy
Animation of an Emerging Star Cluster in WLM Dwarf Irregular Galaxymore_horiz
Radio imaging with the Very Large Array (VLA) captures newborn massive star clusters as they emerge from their birth material in the galaxy NGC 4449. These "super star clusters" contain tens to hundreds of thousands of stars. The young stars produce hot ionized gas which is detectable at radio wavelengths, shown in red here. An image from the Hubble Space Telescope shows the visible starlight in gold.
Making Stars in NGC 4449more_horiz
NGC 253
ALMA Sees Starbursting Clouds Inside NGC 253more_horiz
Molecular gas in the Antennae Galaxies
ALMA Discovers Proto Super Star Clustermore_horiz
Showing images 1 - 6 of 6

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