NGC 1929 is a star
cluster rooted in the nebula N44, Which is found in the Large Magellan Cloud.Massive
stars in the cluster produces powerful radiation, expel matter at high speeds,
and explode as supernovas Relatively Quickly. Winds from the massive stars and supernova
shocks from carve out "superbubbles" in the gas seen in X-rays by
Chandra (blue). Infrared data show dust (red) and cooler gas and optical light
(yellow) Reveals where ultraviolet radiation is Causing the gas to glow.
This composite image
shows a superbubble in the Large Magellan Cloud (LMC), a small satellite galaxy
of the Milky Way, located About 160.000 light years from Earth.
