Table 1.

Physical parameters of the circumnuclear disk and tidally disrupted molecular clouds.

Objectτ(CS 2–1)M  LTE(CS 2–1)*M  LTE(H13CO+)M  LTE(CS 7–6)
[M][M][M]
CND∼0.633.1 × 104(Tex/200)1.5 × 104(Tex/200)1.5 × 104(Tex/22)
Anomaly A∼1.51.3 × 104(Tex/200)2.3 × 103(Tex/200)
Anomaly B∼0.187.0 × 103(Tex/200)2.7 × 103(Tex/200)
Anomaly C∼3.21.0 × 103(Tex/200)
Objectτ(CS 2–1)M  LTE(CS 2–1)*M  LTE(H13CO+)M  LTE(CS 7–6)
[M][M][M]
CND∼0.633.1 × 104(Tex/200)1.5 × 104(Tex/200)1.5 × 104(Tex/22)
Anomaly A∼1.51.3 × 104(Tex/200)2.3 × 103(Tex/200)
Anomaly B∼0.187.0 × 103(Tex/200)2.7 × 103(Tex/200)
Anomaly C∼3.21.0 × 103(Tex/200)

*We assumed A21 = 2.2 × 10−5 s−1 and X(CS) = 1 × 10−8.

We assumed A10 = 3.9 × 10−5 s−1 and X(H13CO+) = 4 × 10−10 (Amo-Baladrón et al. 2011).

We assumed A76 = 0.8 × 10−3 s−1 and X(CS) = 1 × 10−8.

Table 1.

Physical parameters of the circumnuclear disk and tidally disrupted molecular clouds.

Objectτ(CS 2–1)M  LTE(CS 2–1)*M  LTE(H13CO+)M  LTE(CS 7–6)
[M][M][M]
CND∼0.633.1 × 104(Tex/200)1.5 × 104(Tex/200)1.5 × 104(Tex/22)
Anomaly A∼1.51.3 × 104(Tex/200)2.3 × 103(Tex/200)
Anomaly B∼0.187.0 × 103(Tex/200)2.7 × 103(Tex/200)
Anomaly C∼3.21.0 × 103(Tex/200)
Objectτ(CS 2–1)M  LTE(CS 2–1)*M  LTE(H13CO+)M  LTE(CS 7–6)
[M][M][M]
CND∼0.633.1 × 104(Tex/200)1.5 × 104(Tex/200)1.5 × 104(Tex/22)
Anomaly A∼1.51.3 × 104(Tex/200)2.3 × 103(Tex/200)
Anomaly B∼0.187.0 × 103(Tex/200)2.7 × 103(Tex/200)
Anomaly C∼3.21.0 × 103(Tex/200)

*We assumed A21 = 2.2 × 10−5 s−1 and X(CS) = 1 × 10−8.

We assumed A10 = 3.9 × 10−5 s−1 and X(H13CO+) = 4 × 10−10 (Amo-Baladrón et al. 2011).

We assumed A76 = 0.8 × 10−3 s−1 and X(CS) = 1 × 10−8.

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