Table 6
Data for the molecular gas and SFR for a sample of TDGs.
| Name | Dist | FWHM | Area | Mmol | SFR | Ref. |
| [Mpc] | [′′/kpc] | [kpc2] | [107M⊙] | [10-2M⊙ yr-1] | ||
|
|
||||||
| Arp158 | 62.1 | 22/6.6 | 49.3 | 8.5 | 5.0 | (1) |
| Arp105S | 115.0 | 22/12.2 | 169.9 | 19.8 | 8.1 | (2) |
| NGC4676N | 90.0 | 22/9.6 | 201.5 | 10.3 | 8.1 | (2) |
| NGC7252W | 64.0 | 11/3.3 | 12.6 | 1.3 | 0.5 | (2) |
| SQB | 85.0 | 22/10.0 | 112.2 | 48.3 | 32.2 | (2,3) |
| SQB | 85.0 | 4/ 1.6 | 21.2 | 34.0 | 30.0 | (4) |
| SQtip | 85.0 | 4/1.6 | 5.0 | 11.0 | 5.0 | (4) |
| J1032+1952 | 20.4 | 22/2.2 | 6.0 | 10.5 | 2.4 | (5) |
| Arp245N | 31.0 | 22/3.3 | 27.0 | 19.0 | 9.0 | (6,7) |
| VCC 2062 (NE) | 17 | 22/1.8 | 7 | 2.3 | 0.2 | (8,9) |
| VCC 2062 (total) | 17 | 22/1.8 | 2.7 | 1.4 | 0.2 | (8,9) |
Notes. All data are adapted to include He in the molecular gas mass and to a Kroupa IMF. The SFR is mostly derived from Hα except for Arp 158 where it is derived from FUV and 24 μm. The area denotes the area over which the Mmol and SFR have been determined which can be larger than the resolution of the observation.
Reference. (1) Boquien et al. (2011); (2) Braine et al. (2001; Table 2) and reference therein; (3) Lisenfeld et al. (2002a); (4) Lisenfeld et al. (2004); (5) Lisenfeld et al. (2008); (6) Braine et al. (2000); (7) Duc et al. (2000); (8) Duc et al. (2007) (for the CO from IRAM 30 m); (9) this paper (for the SFR).
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