Surveying the Giant H II Regions of the Milky Way with SOFIA. VII. Galactic Center Regions Sgr B1, Sgr B2, and Sgr C

April 2025 • 2025ApJ...983...66D

Authors • De Buizer, James M. • Lim, Wanggi • Radomski, James T. • Karnath, Nicole

Abstract • This study examines the mid-infrared properties of Giant H II (GH II) regions in the Milky Way's Central Molecular Zone (CMZ)—Sgr B1, Sgr B2, and Sgr C—using SOFIA-FORCAST imaging at 25 and 37 μm. It compares these mid-infrared data with previous multiwavelength observations to explore their present star formation activity and global properties. The study identifies 77 massive young stellar object (MYSO) candidates in and around the three regions. Sgr B2 appears to host the youngest MYSOs and have much higher extinction than the other regions, containing several radio sources not detected in the mid-infrared even at 37 μm. Meanwhile, cm radio continuum regions of Sgr B1 shows remarkable correspondence to its mid-infrared emission. Sgr C has fewer confirmed MYSOs, and it seems to have a higher fraction of low-mass young stellar objects and contamination from more evolved interloper/foreground stars. Derived MYSO densities are consistent with GH II regions elsewhere in the Galactic plane, though the CMZ GH II regions appear to have less prolific present star formation overall. Unlike Sgr B2, the cm continuum emission in Sgr B1 and Sgr C GH II regions appears to be absent cold dust and molecular gas, suggesting environmental differences, possibly driven by turbulence and rapid dynamical changes near the Galactic center. Furthermore, unlike typical GH II regions, Sgr B1 and Sgr C are significantly ionized by evolved interloper stars, which likely did not form within these regions. In these ways, Sgr B1 and Sgr C deviate from classical GH II region behavior, thus potentially representing a new category of GH II region or challenging their classification as GH II regions.

Links

• PDF https://iopscience.iop.org/article/10.3847/1538-4357/adbbd9/pdf
• PREPRINT http://arxiv.org/abs/2502.20506
• ELECTR https://iopscience.iop.org/article/10.3847/1538-4357/adbbd9/pdf