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Table 1

CO (J = 3–2) line absorption velocity components toward Sgr A* continuum source and estimated column densities.

(km s−1) Widtha, Δ v (km s−1) Depth, τabs, CO 3−2 Nabs (CO)b (cm−2) N(H2)c (cm−2) Componentd
−315 ± 3 3 ± 1 0.009 1.27 × 1015 3.17 × 1019 New. ENVG. Near Sgr A*?
−264 ± 1 11 ± 1 0.053 2.89 × 1016 7.23 × 1020 New. ENVG. Near Sgr A*?
−198 ± 1 5 ± 3 0.021 4.83 × 1015 1.21 × 1020 HNVG. Foreground cloud
−175 ± 1 11 ± 1 0.086 4.76 × 1016 1.19 × 1021 HNVG. Foreground cloud
−145 ± 2 4 ± 1 0.269 4.91 × 1016 1.23 × 1021 Foreground gas around GC?
−135 ± 2 7 ± 2 1.309 4.33 × 1017 1.08 × 1022 Foreground gas around GC
−121 ± 2 6 ± 2 0.269 8.48 × 1016 2.12 × 1021 Foreground gas around GC?
−73 ± 1 5 ± 1 0.842 2.09 × 1017 5.22 × 1021 CND?
−53 ± 1 6 ± 1 ≫1 3-kpc arm feature
−31 ± 1 5 ± 1 ≫1 −30 km s−1 or 4-kpc arm
−7 ± 1 19 ± 1 ≫1 Galactic arms
12 ± 1 16 ± 1 ≫1 Galactic arms
37 ± 1 21 ± 1 ≫1 GC clouds
50 ± 1 5 ± 1 0.734 1.76 × 1017 4.41 × 1021 GC clouds
61 ± 1 8 ± 1 2.523 1.01 × 1018 2.54 × 1022 GC clouds

Notes. (a) From a multigaussian fit to the 1″-resolution spectrum toward Sgr A*. (b) Assuming Trot (CO) = 5 K. (c) Assuming N(CO)/N(H2) = 4 × 10−5. (d) ENVG = extreme negative velocity gas, HNVG = high negative velocity gas, GC = Galactic center, CND = circumnuclear disk.

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