The CO (J=2-1) distribution in the inner 10 pc of the galaxy

Details The CO (J=2-1) distribution in the inner 10 pc of the galaxy The CO (J=2-1) distribution in the inner 10 pc of the galaxy

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aipc..155..110f&link_type=abstract

AIP Conference Proceedings, Volume 155, pp. 110-113 (1987).

Physics

2

Scientific paper

We report observational results of the J=2-1 CO emission in the 5'×5' region toward Sgr A*. The fully sampled high angular resolution (30`) data reveal considerable details of the neutral gas ``disk'' in the central 10pc of the Galaxy. Although the CO distribution is generally consistent with a tilted rotating disk, the present data indicate that the distribution is significantly asymmetric with respect to Sgr A*. The Co rotation curve derived from the negative velocity CO lobe indicates that the mass in the inner 10pc increases linearly with radius from 3pc to 10pc.

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