Year: 2017
Type: article
Abstract: We present the first systematic study of the density structure of clouds found in a complete sample covering all major molecular clouds in the central molecular zone (CMZ; inner ~200 pc) of the Milky Way. This is made possible with data from the Galactic Center Molecular Cloud Survey (GCMS), which is the first study resolving all major molecular clouds in the CMZ at interferometer angular resolution. We find that many CMZ molecular clouds have unusually shallow density gradients compared to regions elsewhere in the Milky Way. This is possibly a consequence of weak gravitational binding of the clouds. The resulting relative absence of dense gas on spatial scales ~0.1 pc is probably one of the reasons why star formation (SF) in dense gas of the CMZ is suppressed by a factor ~10, compared to solar neighborhood clouds. Another factor suppressing star formation is the high SF density threshold that likely results from the observed gas kinematics. Further, it is possible but not certain that the star formation activity and cloud density structure evolve systematically as clouds orbit the CMZ.
Source: Astronomy and Astrophysics
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Awards: STAR FORMATION TYPICALLY BEGINS IN COLD, DARK CLOUDS THAT ARE NOT SPHERICALLY SYMMETRIC, BUT ELONGATED AS INFRARED DARK CLOUDS OR LONG LINEAR FILAMEN, WE PROPOSE TO ADDRESS THE PROBLEM OF DETERMINING THE STAR FORMATION CHARACTERISTICS OF CLUSTERED OBJECTS IN BLENDED OR UNRESOLVED REGIONS BY COMBININ, G7501114982
OpenAlex ID: W4294939357