S[CLC]i[/CLC]O Emission from the Galactic Center Molecular Clouds

Abstract

We have mapped the J = 1 --> 0 line of SiO in a 1° × 12' (l × b) region around the Galactic center (GC) with an angular resolution of 2' (~4 pc). In contrast to the spatial distribution of other high dipole moment molecules like CS, whose emission is nearly uniform, the SiO emission is very fragmented, and it is associated with some molecular clouds only. In particular, it is remarkable that the SiO emission follows closely the nonthermal radio arc in the GC. The SiO clouds are more extended than the beam, with typical sizes between 4 and 20 pc. High angular resolution (26") mapping in the J = 2 --> 1 line of SiO toward the molecular clouds in Sgr B2 and Sgr A shows that the SiO emission is relatively smooth, with structures of typically 2 pc. From the line intensities of the J = 2 --> 1, J = 3 --> 2, and J = 5 --> 4 transitions of SiO, we derive H2 densities for these clouds of a few 104 cm-3. The SiO fractional abundances are ~10-9 for the SiO clouds and