Young stars enveloped in a transformative cocoon of gas shine brightly in a new image from the Hubble Space Telescope.
The newborn stars belong to a cluster known as NGC 460, which is located in a region of the Small Magellanic Cloud, a dwarf galaxy that orbits the Milky Way. NGC 460 is surrounded by a number of other young stellar clusters and varying sized nebulae, which are clouds of gas and dust that fuel new star formation.
Within this region, also known as N83, there are a number of O-type stars, the brightest, hottest and most massive of main-sequence stars (like the sun), which burn hydrogen at their core. O-type stars are rare; there are thought to be just 20,000 of them in the Milky Way, according to a statement from NASA releasing the Hubble image on March 8.
Source: www.space.com
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