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Table 3.

Model gas masses in the gas tail of ESO 137−001.

Disk CNM (a) Tail CNM (a) Tail WNM (b) Tail WIM Tail HIM SFRdisk/SFRtail
(108 M) (108 M) (108 M) (108 M) (108 M)
Observed 7 9 2 10 2.0
Model A 5.8 4.3 5.0 0.9 4.1 1.2
Model B 7.8 0.4 2.8 0.8 2.5 6.9
Model C 7.0 1.2 2.7 2.2 5.9 5.4

Notes.

(a)

The division between tail and disk region is at x = 2 kpc.

(b)

H I contained in the maps of Fig. 13.

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