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Astronomers have a wide, never wide, never, which never, across hundreds of light years, our galaxy is roaming in the cool, dark, starless South. It has been dubbed Midpoint Cloud and has been identified using the Green Bank telescope. It seems that the dense clouds of the material are channels in the heart of our galaxy. It ports active areas full of dense dust lanes and stars. These lanes can bring twisted substances to the central bar of the Galaxy, and create how stars are created in this extreme environment and offer a rare snapshot of the first stages of the galaxy evolution.

The newly found midpoint cloud can prove to be the key to the structure of the star in the core part of the Akashinga

According to StudyResearchers from the National Radio astronomy Observatory and Green Bank Observatory confirmed the size and shape of GMC, based on density and movement. The gas chaos in the cloud is a mirror of a caustic turmoil in the center of the galaxy, which measures a stupid item that says something about a 200 -year -old era. It can be a comfortable link like our own skyk’s disk field, which is mainly suffering from destruction.

Probably synonymous with gas ChannelsIn the mid -point cloud, a thick dust lane can supply the central wire bar piece with fresh gas, once again supports the interpretation that the formation of the star in the region is prevented from the potential of gravity. But regions like mid -point can collect so many thick gas, which produces new stars.

The team ranked the knot as a compact gas clump, whose material was eliminated inside the cloud by both star radiation and a available, or microwave emission. Supernova’s blasts suggest a shell before a feature, such as massive stars deaths in the region.

Green Bank Observatory Mid -Point Cloud Larry Morgan, a valuable indication of our knowledge, is how the galaxies develop near their centers and form stars. This detection can give scientists a way to know how the matter across the universe flows inside, a hidden cloud at a time.