Co/ Observations of High Negative Velocity Gas Towards the Galactic Centre

Details Co/ Observations of High Negative Velocity Gas Towards the Galactic Centre Co/ Observations of High Negative Velocity Gas Towards the Galactic Centre

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.269..619m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 269, NO. 3/AUG1, P. 619, 1994

Astronomy and Astrophysics

Astronomy

3

Scientific paper

We present CO observations of high negative velocity gas seen towards the Galactic Centre. Two components of this gas are discussed: an east-west ridge centred at -190 km 1; and extended widespread material at under -170 km 1 which forms northeast-southwest ridges. The physical conditions of the -190 km 1 gas are estimated using four CO lines. We associate the -190 km 1 and lower velocity gas with the large-scale Galactic gas distribution. Key words: ISM: clouds - ISM: molecules - ISM: structure - Galaxy: centre - radio lines: ISM.

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