Dense gas dynamics in the Galactic center

Details Dense gas dynamics in the Galactic center Dense gas dynamics in the Galactic center

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..317r&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Physics

Ism, Galactic Center, Infrared

Scientific paper

We have undertaken a survey of dense gas (CS and SiO) in the different kinematic components of the Galactic center (GC) with the aim of studying the physical properties of the high velocity gas and to investigate the possible links between the typical physical conditions of the GC clouds and the global gas dynamics. We have detected dense gas in all the velocity components. The highest SiO/CS ratios are measured towards the Clump 2 and the l = 1.3° complexes. We will discuss the implications of these findings in the context of the GC gas dynamics.

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