Table 2.
Physical properties of the stripped gas and dust extending beyond the optical disc.
| ID | σ100 μm | σ160 μm | S250 μm | SHI | Mdust | MHI |
|---|---|---|---|---|---|---|
| (mJy) | (mJy) | (mJy) | (Jy km s−1) | (M⊙) | (M⊙) | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| NGC 4330 | 18.4 | 16.7 | 18.0 ± 4.7 | 0.1 ± 0.01 | 3.9 ± 1.0 e+4 | 6.3 ± 0.4 e+06 |
| NGC 4522 | 26.0 | 22.0 | 29.8 ± 6.1 | 0.5 ± 0.03 | 6.4 ± 1.3 e+4 | 3.5 ± 0.2 e+07 |
| NGC 4654 | 230.5 | 183.4 | 530.1 ± 39.4 | 17.7 ± 0.6 | 11.4 ± 0.8 e+5 | 1.1 ± 0.1 e+09 |
Notes. Column 1: Galaxy name. Columns 2 and 3: 1σ uncertainty on the FIR 100 μm and 160 μm flux densities within the examined regions. Columns 4 and 5: FIR 250 μm and HI flux densities within the examined regions. Column 6: Dust mass computed from Col. 3 via Eq. (1), assuming a dust temperature of T = 20 K. Column 7: mass of the atomic gas computed from Col. 4 via Eq. (3).
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