Our galaxy and many of the galaxies we observe where star birth is still happening, contain a large number of blue supergiant stars.
While we know a fair amount about how stars are formed, and can even see them forming in many nebulas in our galaxy, what leads to a star being a giant blue main sequence star rather than a smaller longer lived A, F, G, K, M type star (our Sun is G type) is not wholly understood, however new work done at the Instituto de Astrofísica de Canarias think the clue could be in the partners these stars have.
Most star systems are binary star systems, other stars that orbit alongside in various configurations. However, most O and B type stars, the blue giants, are mostly devoid of companions.
The team involve believe this is because during birth, binary partners ended up merging and forming these massive blue stars.
Blue giants are the rock stars of the universe, they live short and energetic lives, and often end in a supernova or even collapsing into stellar black holes. You'll not see these in elliptical galaxies where almost all star birth has ended, but even in the oldest parts of our galaxy, the central bulge, blue giants are being created, and look amazing against the more creamy colour of smaller M, K and G type stars that can live for 10+ billion years, and make their way to the centre still within their main sequence life.
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An international piece of research, led by the Instituto de Astrofísica de Canarias (IAC) has found clues to the nature of some of the brigh








