Star formation sites toward the Galactic center region

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 (|� | �> 345 ◦ , |b| � >345 ◦ , |b| < 2 ◦ ). We fi nd no signif icant difference between the correlation rate of CH3OH masers with green sources in the CMZ and the disk. This suggests that although the physical conditions of the gas are different in the CMZ from that of the Galactic disk, once gravitational instability sets in at sufficiently high densities, signatures of star formation appear to be similar in both regions. Moreover, the detection of green sources, even at the distance of the Galactic center, shows that our technique can easily identify the early stages of star formation, especially in lowextinction regions of the Galaxy. Through the association of H2 Oa nd CH 3OH masers, we identify 15 star-forming sites in the CMZ. We find a higher correlation rate of coincident H2 Oa nd CH 3OH masers within the CMZ compared to the Galactic disk, indicating a difference in the maser evolutionary sequence for star-forming cores in these two regions.