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Disk-Halo interface: The "foot point" of the Galactic Molecular Loops by Riquelme, D.; Amo-Baladron, M. A.; Martin-Pintado, J.; Mauersberger, R.; Bronfman, L.; Martin, S. is a scholarly article available to read on EtoBox.

What is Disk-Halo interface: The "foot point" of the Galactic Molecular Loops about?

We study the disk-halo interaction, in the context of orbits and Giant Molecular loops (GMLs) in the Galactic center (GC) region. We present a large scale survey in the central kpc in SiO(J=2-1), HCO$^+$(J=1-0) and H$^{13}$CO$^+$ (J=1-0), observations in 3mm lines toward a region in two clumps M+5.3-0.3 and M-3.8+0.9 placed in the foot point of two molecular loops, and observations toward selected positions, to trace accretion of the gas from the halo

Author

Riquelme, D.; Amo-Baladron, M. A.; Martin-Pintado, J.; Mauersberger, R.; Bronfman, L.; Martin, S.

Published

2010

Language

EN