Astronomers View Star Formation In The Central Molecular Zone
Recent Galactic plane surveys at a wide range of wavelengths using facilities like the Submillimeter Array and ALMA telescopes have made it possible to study cloud evolution and star formation in the Central Molecular Zone (CMZ), the central 1500 light-years of the Milky Way, whose extreme physical conditions more nearly resemble those at the peak of cosmic star formation. CfA astronomers Eric Keto and Qizhou Zhang and their colleagues carried out a series of computer simulations of massive molecular clouds in a CMZ environment with the goal of characterizing their morphological and kinematic evolution as they orbit the galactic center in this dense, complex region....