Abstract
Aims. We present a study of star formation in the central molecular zone (CMZ) of our Galaxy through the association of three star formation indicators: 6.7 GHz CH3OH masers, 22 GHz H2O masers, and enhanced 4.5 μm emission (‘green’) sources. We explore how star formation in the CMZ(|ℓ| < 1.3°, |b| < 10′) compares with that of the Galactic disk (6 °> ℓ > 345°, |b| < 2°).
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