For decades, astronomers have discovered hundreds of protoplanetary disks—structures believed to represent the early stages of our own solar system. However, most of these discoveries lie within our neighborhood, which may not reflect the extreme conditions found in other parts of the Milky Way.
Among the most dynamic and turbulent regions is the Central Molecular Zone (CMZ) near the Milky Way galactic center, where high pressure and density may shape star and planet formation in fundamentally different ways. Studying protoplanetary systems in the CMZ provides a rare opportunity to test and refine our theories of solar system formation.
An international team of researchers have conducted the most sensitive, highest-resolution, and most complete survey to date of three representative molecular clouds in the Milky Way’s CMZ. Their observations revealed over five hundred dense cores—the sites where stars are being born.